Status Report

NASA ISS On-Orbit Status 4 August 2012

By SpaceRef Editor
August 4, 2012
Filed under , , ,
NASA ISS On-Orbit Status 4 August 2012
http://images.spaceref.com/news/exp32.jpg

All ISS systems continue to function nominally, except those noted previously or below. Saturday – Crew off duty.

At wakeup, Gennady Padalka performed the routine inspection of the SM PSS Caution & Warning panel as part of regular Daily Morning Inspection.

Padalka, Revin, Acaba, Malenchenko, Williams & Hoshide joined in conducting the regular weekly three-hour task of thorough cleaning of their home, including COL (Columbus Orbital Laboratory) and Kibo JPM (JEM Pressurized Module). [“Uborka”, usually done on Saturdays, includes removal of food waste products, cleaning of compartments with vacuum cleaner, damp cleaning of the SM dining table, other frequently touched surfaces and surfaces where trash is collected, as well as the sleep stations with a standard cleaning solution; also, fan screens and grilles are cleaned to avoid temperature rises. Special cleaning is also done every 90 days on the HEPA (high-efficiency particulate air) bacteria filters in the Lab.]

As part of Uborka house cleaning, Sergei, Yuri & Gennady also completed regular weekly maintenance inspection & cleaning of fan screens in the FGB (TsV2) plus Group E fan grilles in the SM (VPkhO, FS5, FS6, VP), and the grilles of the BMP Harmful Contaminants Removal System and SKV air conditioner in the SM.

Joe conducted the regular (~weekly) inspection & maintenance, as required, of the CGBA-4 (Commercial Generic Bioprocessing Apparatus 4) and CGBA-5 payloads in their ERs (EXPRESS Racks) at Lab O2 & O1, focusing on cleaning the muffler air intakes.

Akihiko filled out his standard FFQ (Food Frequency Questionnaire) on the MDLT (Medical Laptop). It was Aki’s 3rd. [On the FFQs, USOS astronauts keep a personalized log of their nutritional intake over time on special MDLT software. Recorded are the amounts consumed during the past week of such food items as beverages, cereals, grains, eggs, breads, snacks, sweets, fruit, beans, soup, vegetables, dairy, fish, meat, chicken, sauces & spreads, and vitamins. The FFQ is performed once a week to estimate nutrient intake from the previous week and to give recommendations to ground specialists that help maintain optimal crew health. Weekly estimation has been verified to be reliable enough that nutrients do not need to be tracked daily.]

Afterwards, Hoshide completed Part 2 of the TCA-L PPA (Thermal Control Assembly for Low Temperature Loop / Pump Package Assembly) replacement in the JAXA JPM (JEM Pressurized Module) which he performed successfully yesterday. Today, the worksite was closed out, cleaned up and the removed PPA attached to the PPA FSE (Flight Support Equipment).

Sergei Revin conducted the routine daily servicing of the SOZh system (Environment Control & Life Support System, ECLSS) in the SM. [Regular daily SOZh maintenance consists, among else, of checking the ASU toilet facilities, replacement of the KTO & KBO solid waste containers, replacement of EDV-SV waste water and EDV-U urine containers and filling EDV-SV, KOV (for Elektron), EDV-ZV & EDV on RP flow regulator.]

At ~8:40am EDT, the entire crew held the regular WPC (Weekly Planning Conference) with the ground, discussing next week’s “Look-Ahead Plan” (prepared jointly by MCC-H and TsUP-Moscow timeline planners), via S-band/audio, reviewing upcoming activities and any concerns about future on-orbit events.

At ~2:35pm, Suni Williams is scheduled for her weekly PFC (Private Family Conference), via S-band/audio and Ku-band/MS-NetMeeting application (which displays the uplinked ground video on an SSC laptop).

The crew worked out on the TVIS treadmill with vibration isolation & stabilization (CDR, FE-2, FE-4), ARED advanced resistive exerciser (CDR, FE-3, FE-5, FE-6), T2/COLBERT advanced treadmill (FE-3, FE-5, FE-6), and VELO ergometer bike with load trainer (FE-2, FE-4).

Suni conducted her session on the T2/COLBERT advanced treadmill with the Treadmill Kinematics protocol, setting up the HD camcorder in Node-1, placing tape markers on her body, recording a calibration card in the FOV (Field of View) and then conducting the workout run within a specified speed range. The video will be downlinked via MPC (Multi-Protocol Converter). [Purpose of the Kinematics T2 experiment is to collect quantitative data by motion capture from which to assess current exercise prescriptions for participating ISS crewmembers. Detailed biomechanical analyses of locomotion will be used to determine if biomechanics differ between normal and microgravity environments and to determine how combinations of external loads and exercise speed influence joint loading during in-flight treadmill exercise. Such biomechanical analyses will aid in understanding potential differences in gait motion and allow for model-based determination of joint & muscle forces during exercise. The data will be used to characterize differences in specific bone and muscle loading during locomotion in the two gravitational conditions. By understanding these mechanisms, appropriate exercise prescriptions can be developed that address deficiencies.]

Tasks listed for Revin, Malenchenko & Padalka on the Russian discretionary “time permitting” job for today were –
* A ~30-min. session for Russia’s EKON Environmental Safety Agency, making observations and taking KPT-3 aerial photography of environmental conditions on Earth using the NIKON D3X camera with the RSK-1 laptop, and
* More preparation & downlinking of reportages (written text, photos, videos) for the Roskosmos website to promote Russia’s manned space program (max. file size 500 Mb).

Weekly Science Update (Expedition Thirty-Two – Week 5).

2D NANO Template (JAXA): Mission completed.

3D SPACE: Complete.

ACE (Advanced Colloids Experiment, NASA): “Joe – Excellent job photo documenting and video recording each of the five ACE Samples. The image data you gathered for us was exactly what we needed to decide which ACE Sample to investigate first. The PI looked for the sample that has the fewest or smallest bubble(s) in its sample wells (i.e. the sample with the best chance of being mixed well). Bubbles prohibit the rotation of the stir bars in the well. Suni – Thank you for your hard work to configure LMM for ACE and installing the ACE Sample S/N 2003. We especially appreciate the time and care you took with mixing the sample. Your diligence paid off! Using the LMM Microscope from the ground, we have determined that the sample wells were successfully mixed (i.e. the microparticles are suspended in the fluid). We powered up FIR and LMM shortly after Suni closed the rack doors. We are currently running nine days of continuous operations to investigate how the various microparticles in this sample behave. We are successfully collecting data but have yet to analyze any data.”

ALTCRISS (Alteino Long Term monitoring of Cosmic Rays on the ISS): Complete.

ALTEA SHIELD Shielding (NASA/ASI): On GMT160, Andre Kuipers successfully relocated the ALTEA instrument from Destiny to Columbus. He reconfigured the instrument in the so-called “shielding” configuration. The first measurement session has started right away, aiming at characterizing dedicated shielding tiles. On GMT201, one of the Silicon Detector Units (SDU #1) went off. This was recovered by a crew activity on GMT202. However on GMT202, SDU#2, which is the reference detector without shielding tiles, went off. Since this removes the comparison reference for the detectors with shielding tiles, this has science impact. Thank you, Joe, for performing the associated recovery activity on GMT209. Since then data from all 3 SDU’s are being received again. To date, around 47 cumulative days of measurements have been performed. Session#1 must be pursued for a minimum of 40-60 cumulative days, hence the minimum required duration on the first location has been met. [Cosmic radiation consists of very small, atomic-sized particles that are flying around in space at tremendous speeds. Their energy is so high that these particles, like tiny bullets, can permeate through the complete structure of the ISS. Exposure of astronauts to cosmic radiation is risky from a medical point of view. The best way to protect our astronauts against cosmic radiation is to build the complete ISS from lead! This would solve the problem but the enormous mass can impossibly be launched into space. Therefore different materials, much lighter than lead, are being tested to be used as shielding materials. Two of those will be investigated in the ALTEA-SHIELD experiment. The effectiveness of the shielding materials will be measured on board by a set of special radiation detectors. Some detectors will be covered with tiles made of shielding materials, some others will not. We are looking forward to find out what difference it will make!”]

Amine Swingbed (NASA): No report.

AMS-02 (Alpha Magnetic Spectrometer): No report.

APEX (Advanced Plant Experiments on Orbit) -Cambium: No report.

APEX-TAGES (Transgenic Arabidopsis Gene Expression System): No report.

Asian Seed 2010 (JAXA): Returned on ULF6.

BASS (Burning and Suppression of Solids, NASA): We have not performed operations this week. We are still working on getting additional igniters up to ISS and it looks like this will be done by October. This will be fine with us since we have a break in our test operations for several months to make room in the MSG for another investigation. We will have one more day of operations (and perhaps up to two more) in August before this break. In the meantime, we are continuing analysis of the data obtained so far. We have been looking at the effect of nitrogen extinguishment on the flames. It turns out that for our experiment if the flame is allowed to burn too long it becomes strong enough that our maximum nitrogen supply rate (0.5 liters per minute) is not able to completely extinguish the flame. But if the flame has not been allowed to burn for as long a time then the nitrogen can put it out.

BCAT-6 (Binary Colloidal Alloy Test 6): “Many thanks for taking the time to review in detail the information package on BCAT-C1. The questions asked reflect a deep understanding of the issues and the differences between BCAT-C1 and the previous versions, and an acute concern for details. The ground team is eager to begin operations and is thrilled by your participation. Good luck next week. [Colloids are particles as small as a few tens of nanometers (a thousandth of a thousandth of a millimeter) that are suspended in a medium, usually a liquid or a gas. The name “colloid” comes from the Greek word for “glue”, and expresses very important properties of colloids: when small and light enough, particles can be influenced in their behavior by forces of electromagnetic origin, and make them stick together, or repel each other depending on the configuration. Colloids are widely studied in science because the forces between particles can be controlled and tuned and because particles, while being small enough to be influenced by such forces, are big and slow enough to be seen with a relatively simple and inexpensive laboratory instrument like a microscope. This is why colloids are often studied as model for molecular systems (like standard gases or liquids) where molecules, the individual constituents, are much smaller than colloids and cannot be seen with light. As mentioned, forces between colloids can be tuned giving rise to a rich variety of phenomena. One of them is aggregation, which is when particles stick together and tend to form structures. Among the many ways to induce particle aggregation, one allows to do so by controlling the temperature of the solution in which the particles are immersed, thanks to very weak forces called “critical Casimir forces” that have been predicted more than 30 years ago but just partially verified in experiments. The objective of SODI COLLOID is to measure such forces and produce a controlled aggregation of tiny plastic particles. This would allow to shed light on critical Casimir forces and to make a step towards the fabrication of new nanostructured materials with remarkable optical properties for industrial applications.]

BLB (Biolab, ESA): No report.

BIORHYTHMS (JAXA, Biological Rhythms): No report.

BISE (CSA, Bodies in the Space Environment): No report.

BISPHOSPHONATES: No report.

BXF-Facility (Boiling eXperiment Facility, NASA): No report.

BXF-MABE (Microheater Array Boiling Experiment, NASA): No report.

BXF-NPBX (Pool Boiling Experiment, NASA): No report.

CARD (Long Term Microgravity Model for Investigating Mechanisms of Heart Disease, ESA): No report.

CARDIOCOG-2: Complete.

CB (JAXA Clean Bench): No report.

CBEF-2 (JAXA Cell Biology Experiment Facility)/SPACE SEED: No report.

CCISS (Cardiovascular & Cerebrovascular Control on Return from ISS): No report.

CERISE (JAXA): No report.

CCF (Capillary Channel Flow, NASA): No report.

CFE-2 (Capillary Flow Experiment 2, NASA): “Joe: Thanks for another great run on Vane Gap 2 (VG2). Filling the vane perforations can be a challenge. You were able to fill the perforations and remove the residual fluid from the vane easily and efficiently. We were happy to see the wetting and de-wetting events along with the bulk shift for VG2. Thank you for your flexibility to find the critical vane angles. Also, your description of the de-wetting events that occurred during LOS was exactly what we needed. We look forward to working with you again.”

CFS-A (Colored Fungi in Space-A, ESA): No report.

CSI-5/CGBA-5 (CGBA Science Insert #5/Commercial Generic Bioprocessing Apparatus 5): No report.

CGBA-2 (Commercial Generic Bioprocessing Apparatus 2): Complete.

CIR (Combustion Integrated Rack), MDCA/Flex: No report.

CIRCADIAN RHYTHMS (ESA): “Thank you Aki for performing the very first ever on-orbit CIRCADIAN RHYTHMS measurement session from the evening of GMT212 until morning of GMT214. Science data assessment will be done upon Portable PFS downlink after VO2max session on GMT221. We are very grateful for your help to start this new ESA science experiment!”

Commercial (Inc 23&24, JAXA): No report.

Commercial (Inc 25 & 26, JAXA): No report.

CSAC (Chip-Scale Atomic Clock, SPHERES): No report.

CSLM-2 (Coarsening in Solid-Liquid Mixtures 2): No report.

CsPins (JAXA): No report.

CubeLab: No report.

CW/CR (Cell Wall/Resist Wall) in EMCS (European Modular Cultivation System): Complete.

DECLIC-ALI (Device for the Study of Critical Liquids & Crystallization-ALICE-like, CNES/NASA): No activity for this week. DECLIC is off until GMT 247. Scientists are developing the work program of the next sequence (ALI-SC8).

DomeGene (JAXA): Complete.

DOSIS (Dose Distribution Inside ISS, ESA): Nominal science acquisition with active and passive dosimeters inside Columbus.

EarthKAM (Earth Knowledge Acquired by Middle School Students): No report.

EDR (European Drawer Rack, ESA): No report.

EKE (Endurance Capacity by Gas Exchange and Heart Rate Kinetics During Physical Training, ESA): No report.

ELITE-S2 (Elaboratore Immagini Televisive – Space 2): Planned.

EMCS (European Modular Cultivation System): “Thanks, Andre, for your help with the EMCS Relief Valves check.”

ENERGY (ESA): No report. [Background: In the ENERGY experiment, astronauts are invited to participate in a study that aimed to evaluate how much food is needed for astronauts during long-term space missions. To do so, the science team will measure every component or variable of the astronaut’s energy expenditure reflecting his energy needs. Those variables will be measured twice: up to 4 months before flight and after at least 3 months in space but 3 weeks before landing. The changes in the astronaut’s energy balance and expenditure will be measured, which will help in deriving an equation for energy requirements in weightlessness. This will contribute to planning adequate, but not excessive cargo supplies for food.]

ENose (Electronic Nose): No report.

EPM (European Physiology Module): Rack activated in support of ENERGY armband data transfers.

EPO (Educational Payload Operations, NASA) (Eye in the Sky; Sleep 2): No report.

EPO (Educational Payload Operations, NASA) (Sesame Street): No report.

EPO (Educational Payload Operations, NASA) (Kids in Micro-G): No report.

EPO (Educational Payload Operations, NASA) (Earth/Moon/Mars Demo): No report.

EPO (Educational Payload Operations, NASA) (Space Sports): No report.

EPO (Educational Payload Operations, NASA) (ISS Orbit): No report.

EPO (Educational Payload Operations, ESA): No report.

EPO CONVECTIONS (ESA): “No report.

EPO MISSION X (ESA): No report.

EPO Spaceship Earth (ESA): No report.

EPO LES-2 (ESA): No report.

EPO GREENHOUSE (ESA): No report.

EPO 3-min Video (JAXA): No report.

EPO J-Astro Report (JAXA): No report.

EPO Dewey’s Forest (JAXA): Closed out on 3/15.

EPO Space Clothes (JAXA): Complete.

EPO Hiten (Dance, JAXA): No report.

EPO Lego Bricks (NASA, JAXA): No report.

EPO Moon Score (JAXA): No report.

EPO OpticSphere & ISSOrbit-Demo (NASA): No report.

EPO Kibo Kids Tour (JAXA): Complete.

EPO Paper Craft (Origami, JAXA): No report.

EPO Poem (JAXA): No report.

EPO-5 SpaceBottle (Message in a Bottle, JAXA): No report.

EPO-6 Spiral Top 2 (JAXA): No report.

EPO-7 Doctor Demo (JAXA): No report.

EPO-7 Green Tea Preparation (JAXA): No report.

EPO-7 Ink Ball (JAXA): No report.

EPO-7 Video (JAXA):

EPO-7 Try Zero-G (JAXA): No report.

EPO-8 Space Sakura (JAXA): No report.

EPO-8 Space Musical Instruments (JAXA): No report.

ERB-2 (Erasmus Recording Binocular, ESA): [ERB-2 aims are to develop narrated video material for various PR & educational products & events, including a 3D interior station view.] No report.

ETD (Eye Tracking Device): Completed.

FACET-2 (JAXA): No report.

FERULATE (JAXA): No report.

FIR/LMM/CVB (Fluids Integrated Rack / Light Microscopy Module / Constrained Vapor Bubble): No report.

Fish Scales (JAXA): Completed on FD7/ULF-4 and returned on STS-132.

FOAM STABILITY EPO (ESA): No report.

FOCUS: No report.

FSL (Fluid Science Laboratory, ESA): No report.

FWED (Flywheel Exercise Device, ESA): No report.

GENARA-A (Gravity Regulated Genes in Arabidopsis A/ESA): No report.

GEOFLOW-2 (ESA): Experiment completed! [Background: Everybody is familiar with liquids. In an average day we get to use, handle or drink water or other liquids. And everybody knows how fluids (that is liquids and gases) behave: when subjected to a net force, may be pressure, a temperature difference or gravity, they can move freely. Scientists have been studying how fluids move for centuries, and managed to write mathematical formulas that can describe and predict such movements. Unfortunately, these equations are extremely complex and only approximate solutions are known. As a result, our quantitative understanding of fluid movement is just partial. This is especially true for natural phenomena where the forces can be enormous and unpredictable, like in oceans or in the atmosphere, or the interior of the earth, where rocks are exposed to pressures and temperatures so incredibly high that they slowly move and adapt their shape. That is, over hundreds of years rocks flow just like a very viscous liquid. Scientists try to study such flows but cannot observe them directly due to the fact that they take place deep beneath the surface of our planet. The only way is to have computers simulating those movements starting from the equations, but how to check whether computers are correct? This is what Geoflow II is trying to answer on board the International Space Station. Geoflow II is a miniature planet that has some of its essential ingredients: a fluid can freely move inside a spherical container that rotates, has temperature differences and has a simulated gravity directed towards the centre just like in a real planet. By taking pictures of the fluid movements, scientists are able to understand the essential characteristics of the flows and determine whether computer simulations are correct or whether they need to be refined and improved towards a better understanding of the elusive movements that take place inside our planet.]

HAIR (JAXA): No report.

HDTV System (JAXA): No report.

Hicari (JAXA): No report.

Holter ECG (JAXA): No report.

HQPC (JAXA): No report.

HREP (HICO/Hyperspectral Imager for the Coastal Ocean & RAIDS/Remote Atmospheric & Ionospheric Detection System/JAXA): HICO has taken 6144 images to-date. The most recent HICO images include parts of Australia, Hawaii, South Africa, and the Bahamas. RAIDS is continuing to collect secondary Science data including nighttime atmospheric disk photometry, spectra and temperatures. Extreme Ultra Violet airglow spectroscopy and optical contamination studies will also be performed.

HRF-1 (Human Research Facility 1, NASA): No report.

HydroTropi (Hydrotropism & Auxin-Inducible Gene Expression in Roots Grown under Microgravity Conditions/JAXA): No report.

ICE CRYSTAL (JAXA): Complete.

ICV (Integrated Cardiovascular): “Another great Echo this week! You guys rock! Also, thanks to Joe for working the Cardiopres cuff issue so that data collection could continue. We have not been able to successfully downlink two of Aki’s Holter files despite multiple attempts, so a re-download of those cards is planned for next week when Joe is downloading his ambulatory monitoring data.”

IMMUNO (Neuroendocrine & Immune Responses in Humans During & After Long Term Stay at ISS): No report.

INTEGRATED IMMUNE: No report.

InSPACE-3 (Investigating the Structure of Paramagnetic Aggregates from Colloidal Emulsions 3): Inspection of the vials was completed and pictures are under review by the ground team.

IRIS (Image Reversal in Space, CSA): No report.

ISS Amateur/Ham Radio: No report.

ISSAC (ISS Agricultural Camera, NASA): ISSAC Ops are ongoing and nominal. Special thanks to Joe, Suni, and Aki for their help and support in opening the shutter this week, we captured 13 out of 16 targets. Due to blackout period (Aug 1-16), ISSAC will have no access to US targets, but imaging ops will continue to capture International Disaster Charter (IDC) and secondary targets around the world.

IV Gen (Intravenous Fluids Generation): No report.

JOURNALS (Behavioral Issues Associated with Isolation and Confinement, NASA): No report. [Studies conducted on Earth have shown that analyzing the content of journals and diaries is an effective method for identifying the issues that are most important to a person. The method is based on the reasonable assumption that the frequency that an issue or category of issues is mentioned in a journal reflects the importance of that issue or category to the writer. The tone of each entry (positive, negative, or neutral) and phase of the expedition also are variables of interest. Study results will lead to recommendations for the design of equipment, facilities, procedures, and training to help sustain behavioral adjustment and performance during long-duration space expeditions to the ISS, asteroids, the Moon, Mars, and beyond. Results from this study could help to improve the behavioral performance of people living and working under a variety of conditions here on Earth.]

KID/KUBIK6: No report.

KUBIK 3/6 (ESA): No report.

LMM/PACE-2 (Light Microscopy Module / Preliminary Advanced Colloids Experiment): No report.

LEGO Bricks: “Thanks for your work on the ghost load. This was completed to support our upcoming operations.”

LOCAD-PTS (Lab-on-a-Chip Application Development-Portable Test System): No report.

MAMS (Microgravity Acceleration Measurement System, NASA): No report.

Marangoni Exp. (JAXA): No report.

Marangoni DSD – Dynamic Surf (JAXA): Payload name was change from Marangoni DSD to Dynamic Surf.

Marangoni UVP (JAXA): No report.

MARES (Muscle Atrophy Research & Exercise System, ESA/NASA): No report.

Matryoshka-2 (RSA): No report.

MAXI (Monitor of All-sky X-ray Image, JAXA): External payload. Continuing telemetry monitoring. VSC Imagery was downloaded via ground activity on 7/2 and 7/4. MAXI MRDL data has been back on normal.

MDCA/Flex-2: Last week we reported four MDCA/FLEX-2 Quiescent test points performed on GMT 191. The test points used 100% decane fuel and were performed at a 1.0-atm chamber environment of 14% oxygen and 86% nitrogen. Some surprising observations were made for these test points: Despite the low oxygen concentration (14%) of these test points, we observed sustained combustion for fuel droplets of diameters less than 2.0 mm. We observed radiative extinction for surprisingly small droplet diameters (i.e., around Do = 1.75 mm). Radiative extinction is flame extinction caused by excessive radiative energy loss from the flame, and it occurs at relatively larger droplet and flame sizes. Surprisingly, recent testing performed at lower pressures (i.e., 0.5 atm) and at the same low oxygen concentration (14%) showed longer burning times, by as much as 2-3 times.

MEIS (Marangoni Experiment for ISS) in JAXA FPEF (Fluid Physics Experiment Facility): No report.

MELFI (Minus Eighty Laboratory Freezer for ISS, NASA): “Joe: Thanks for all the effort on the EU R&R. MELFI1 is cooling nominally.”

Microbe-2 (JAXA): Sample returned by ULF6.

Micro-G Clay (JAXA EPO): Complete.

Miscible Fluids in Microgravity (MFMG): No report.

MISSE-8 (Materials ISS Experiment 8): MISSE-8 ReflectArray, HyperX and SEUXSE-II experiments continue with nominal operations. PASCAL is performing nominal commanding that produced IV curves of the solar cells. IV curves are plots of the current versus voltage for solar cells and tell a lot about how these are performing. The SpaceCube experiment is running code for new radiation hardening by software.

MMA (JAXA/Microgravity Measurement Apparatus): No report.

MPAC/SEED (JAXA): No report.

MSG-SAME (Microgravity Science Glovebox-Smoke Aerosol Measurement Experiment): No report.

MSPR (Multi Purpose Small Payload Rack, JAXA): On 6/13, Don completed greasing the QDs of the MSPR Work Volume and Combustion Chamber QD successfully, thank you very much.

MSL (Materials Science Laboratory, ESA): Three processed Sample Cartridge Assemblies (SCA’s) have been returned with SpX-D.

MTR-2 (Russian radiation measurements): Passive dosimeters measurements in DC-1 “Pirs”.

MULTIGEN-1: Completed.

MYCO 3 (JAXA): On 9/22, Mike and Satoshi completed sample collection.

MyoLab (JAXA): Completed on 4/20.

NanoRacks (NASA): No report.

NANOSKELETON (Production of High Performance Nanomaterials in Microgravity, JAXA): No report.

NANO STEP (JAXA): Aki, thank you very much for the cartridge installation of Nano Step on GMT 212. Ground is now performing checkout for the experiment.

NEURORAD (JAXA): No report.

NEUROSPAT (ESA/Study of Spatial Cognition, Novelty Processing and Sensorimotor Integration): No report. [During microgravity stay, the human body goes through multitude of physiological changes in order to accommodate to the new environment. As the brain is a master organ where major crucial processes take place, it is fundamental to understand how it manages adaptation for living in Space. One of the main purposes of Neurospat (NES) experiment is to focus on how microgravity environment influences cerebral activity of astronauts aboard ISS. For this, the global electrical activity of the brain of the astronaut is measured thanks to electroencephalogram (EEG) technique, while he or she is executing specific tasks through a computer as if it was a kind of videogame. In practice, the astronaut is wearing a specially equipped cap with passive, gel filled electrodes that are in contact with his/her scalp while he or she is performing the specific tasks that we have designed. These are visual-orientation perception and visuo-motor tracking tasks that may be encountered on a daily basis. The tasks allow the study of 5 cognitive processes: Perception, Attention, Memorization, Decision and Action. Besides there are also task-irrelevant images that are showed to the astronaut in order to assess how well he or she processes novel visual stimuli. The electrodes all over the scalp are linked to sensitive amplifiers that allow us to measure small variations of electrical potential between different regions of the scalp. These signals are in turn used to estimate activity in the cerebral cortex related to the task being performed. Also, they serve to identify the mental processes associated with these tasks and to localize in the brain the sources of the underlying neural activity. After analysis of the data we can better understand whether the novel environment of microgravity accompanied by a multitude of stressors may place an increased load on the cognitive capacity of the human brain and whether the sensory signals and motor responses of astronauts are processed and interpreted differently because a new reference frame.]

NightPod (ESA): NightPod images have been presented in a news blog on the ESA PromISSe website: http://blogs.esa.int/promisse/2012/04/05/nightpod/

NOA-1/-2 (Nitric Oxide Analyzer, ESA): Complete.

NUTRITION w/REPOSITORY/ProK: “Suni, you’ve successfully completed your activities for Nutrition, Repository and Pro K. We expect that your data will be on the ground later today. Thank you for reporting your barcodes for your blood and urine samples. This helps tremendously with sample return. Your next Pro K session (~FD30) will include a monitored diet session. We look forward to working with you again in the next few weeks. Have a great week.

ODK (Onboard Diagnostic Kit, JAXA): “Aki, thank you very much for the functional checkout of Onboard Diagnostic Kit. All of the functions were confirmed to be fine. “

PADIAC (Pathway Different Activators, ESA): No report.

PADLES (JAXA, Area PADLES 6/7; Passive Area Dosimeter for Lifescience Experiment in Space): The 17 dosimeters installed inside the JEM continue to acquire radiation data. This experiment will continue until 30S return.

PASSAGES (JAXA): No report. [PASSAGES is an experiment about the strategies involved in the perception of the world around us. Seeing correctly the world is necessary to success our gestures, our actions, such as catching a ball, stepping an obstacle on the ground or passing through an opened door. In this experiment, we want to know if the strategies involved on Earth continue to be used when the astronaut is in a weightlessness environment for a long period. To investigate this question, the participant sees 3D scenes on the screen of a laptop such as a video game. The scene is a room with an opening which can vary in width. The task of the participant is to decide if yes or no he or she could pass through the aperture without rotating or scrunching the shoulders. The science team uses typical methods from psychophysics and manipulates several factors to highlight the strategies used by the participant. Then, the science team will compare the performances obtained on ground with those obtained onboard.]

PCDF-PU (Protein Crystallization Diagnostic Facility – Process Unit): No report.

PCG (JAXA, Protein Crystal Growth): Mission completed last week.

PCRF (Protein Crystallization Research Facility) Reconfiguration (JAXA): See PCG.

PLSG (Plant Signaling, NASA/ESA): No report.

PMDIS (Perceptual Motor Deficits in Space): Complete.

POLCA/GRAVIGEN (ESA): Complete.

Portable PFS: “Dear Don and Andre, P-PFS was used for your THERMOLAB sessions on GMT156/157. Please refer to THERMOLAB.”

Pro K: No report.

RadGene & LOH (JAXA): Complete.

RadSilk (JAXA): No report.

Reaction Self Test (RST/Psychomotor Vigilance Self Test on the ISS): “Joe, Suni, and Aki, thank you for your participation in Reaction Self tests, we greatly appreciate all of your efforts!”

Reversible Figures (ESA): No report. [Background: The objective of this study is to understand the relationship between gravity and depth perception. Another objective is to identify the problems associated with depth and distance perception in astronauts with the goal of developing countermeasures to reduce any associated performance alteration. This experiment investigates cases in which what astronauts might think to see, fails to achieve a correct representation of the environment, namely, optical illusions. Ten ambiguous figures, with or without depth cues, are presented to an astronaut in virtual reality goggles. These figures are ambiguous because they can be seen at first sight in two different ways. The figure does not change, but after some time the brain reverses (flip-flops) its interpretation. The astronaut is asked to look closely at each figure and to indicate with a mouse trackball which view he/she sees first, and when the view flip-flops. The interval between the views will be compared between 1g and 0g conditions. In 0g, the astronaut will do the test while free-floating to eliminate all orientation cues. This experiment will be performed three times pre-flight, then up to six times in-flight, and again three times post-flight. The science team will then compare the results of these tests across these gravitational environments. It is expected that the frequency of flip-flops of figures with depth cues will be different in between 0g and 1g, and that an adaptation to long-term exposure to weightlessness, as well as a re-adaptation to Earth gravity, will take place.]

ROALD-2 (Role of Apoptosis in Lymphocyte Depression 2, ESA): No report. [Background: The ROALD-2 experiment studies how the function of T-cells from the immune system are affected by microgravity and spaceflight. T-cells play an important role in controlling the immune systems response to infection. It has previously been shown that the immune response of astronauts can be reduced following spaceflight and it has also been shown that the activation of T-cells in culture is reduced in microgravity. A series of experiments on T-cells and other immune system cells have been previously performed by different scientific teams on Space Shuttle and the ISS over the last 30 years. The data from these individual experiments provides information which together can be used to understand the mechanisms by which gravity or the absence of gravity can affect T-cell function.]

Robonaut (NASA): No report.

RYUTAI Rack (JAXA): No report.

SAIBO Rack (JAXA): No report.

SAMS/MAMS (Space & Microgravity Acceleration Measurement Systems): No report.

SAMPLE: Complete.

SCOF (Solution Crystallization Observation Facility, JAXA): No report.

SEDA-AP (Space Environment Data Acquisition Equipment-Attached Payload, JAXA): Continuing telemetry monitoring.

SHD (Space Headaches, ESA): “Joe, we truly appreciate that you always remember to fill your weekly Space Headaches questionnaire!”. [Background: The neurologists from Leiden University want to study the question whether the astronauts, while in space, suffer from the headaches. With the help of simple questionnaires the astronauts will register the headache episodes and the eventual accompanying symptoms. The results will hopefully help to characterize the frequency and characteristics of space headache and to develop countermeasure to prevent/minimize headache occurrence during the space flight.]

SHERE II (Shear History Extensional Rheology Experiment II): No report.

SLAMMD (Space Linear Acceleration Mass Measurement Device): No report.

SLEEP (Sleep-Wake Actigraphy & Light Exposure during Spaceflight): No report.

SLICE (Structure & Liftoff In Combustion Experiment): No report. [See under BASS.]

SMILES (JAXA): Continuing telemetry monitoring.

SODI/IVIDIL (Selectable Optical Diagnostics Instrument/Influence of Vibration on Diffusion in Liquids, ESA): No report.

SODI/COLLOID (Selectable Optical Diagnostics Instrument/Colloid): No report.

SODI-DSC (Selectable Optical Diagnostics Instrument/Diffusion & Soret Coefficient, ESA): No report. [Background: Fluids and gases are never at rest. This statement is in apparent contradiction with our experience: when we pour water in a glass and wait until all flows have disappeared and the temperature of the liquid is in equilibrium with that of the room, we see that water appears to be completely at rest. However, if we were able to see the individual molecules of water with a very powerful microscope, we would discover that they are incessantly moving and collide with each other following frantic, random paths even if the liquid appears to be quiescent at naked eye. Scientists are interested in observing and measuring such movements because they reveal important, practical information: how fast does heat propagates in a fluid? How fast do liquid mixtures mix? Such phenomena occur in absence of a macroscopic flow, that is when the fluid appears to be at rest, and are called heat and mass diffusion respectively. While the theoretical prediction of heat and mass diffusion is still quite challenging, its measurement is a standard laboratory practice, but may become extremely difficult or impossible when dealing with mixtures of many liquids, due to the fact that such measurement needs to be carried out when the fluid is quiescent, a condition sometimes impossible to achieve on ground. This is precisely the objective of the SODI DSC experiment carried out on board the International Space Station: the measurement of diffusion in mixtures of liquids. By using very sensitive optical techniques, it will be possible to measure mass diffusion, compare with current theories, and improve our present understanding of how molecules move in liquid mixtures. The results will be used by the large team of scientists involved in the project to try to understand which of the many existing theories for mass diffusion is correctly predicting the experimental behavior.]

SOLAR (Solar Monitoring Observatory, ESA): Currently out of Sun Visibility Window (SVW). SOLACES is in heated mode. Next SVW#56 expected to start on GMT230.

SOLO (Sodium Loading in Microgravity): No report.

Space-DRUMS (Space Dynamically Responding Ultrasonic Matrix System): No report.

Space Food (JAXA): No report.

SPHERES (Synchronized Position Hold, Engage, Reorient, Experimental Satellite): No report.

SPHINX (SPaceflight of Huvec: an Integrated eXperiment, ESA): No report.

SPICE (Smoke Point In Co-flow Experiment): No report.

SPINAL (Spinal Elongation): No report.

SPRINT: No report.

SS-HDTV (Super Sensitivity High Definition Camera, JAXA): Mission completed last week.

STP-H3 (Space Test Program – Houston 3): MHTEX is continuing with a test of the Capillary Pumped Loop (CPL) and the CPL is currently in a steady state. VADER continues to characterize the performance of the Aerogel blanket attached to the backside of the experiment. Canary collected data during the 47P re-docking and final undocking events earlier this week. Canary also took data during the 48P docking event. DISC has acquired more images this week and is processing images that were taken in previous weeks.

SWAB (Characterization of Microorganisms & Allergens in Spacecraft): No report.

TASTE IN SPACE (ESA): No report.

THERMOLAB (ESA): No report.

TRAC (Test of Reaction & Adaptation Capabilities): Planned.

TREADMILL KINEMATICS: “Thanks, Joe, for your 3rd Treadmill Kinematics session!”

TRIPLELUX-B (ESA): No report.

ULTRASOUND: Planned.

UMS (Urine Monitoring System (NASA): No report.

VASCULAR (CSA): “Many thanks for recording the Vascular Podcast on Thursday. This video will be watched with interest by the public.”

VCAM (Vehicle Cabin Atmosphere Module, NASA): No report.

VESSEL ID System (ESA): Nominal data acquisition with the NorAIS receiver. [Background: As the ISS circles Earth, it has been tracking individual ships crossing the seas beneath. An investigation hosted by ESA in COL module has been testing the viability of monitoring global maritime traffic from the station’s orbit hundreds of kilometers above since June 2010. The ship-detection system being tested is based on the AIS (Automatic Identification System), the marine equivalent of the air traffic control system. Astronauts were instrumental in enabling the COLAIS experiment, which is an in-orbit demonstration project of ESA’s General Support Technology Program. COL was not originally outfitted with VHF antennas to capture the AIS signals; they were installed on the outside of the module during a spacewalk in November 2009, with the remaining piece of hardware, the ERNOBox control computer, installed inside COL along with the NORAIS receiver in May 2010.- The two operational phases with the first receiver from Norway, or NORAIS, which is operated by FFI/Norway, have been extremely successful, with data telemetry received by the N-USOC, in Trondheim, Norway, via ESA’s COL-CC in Germany. Data has been received by NORAIS in almost continuous operation, and all modes of operation have worked extremely well. On a good day, approximately 400,000 ship position reports are received from more than 22,000 different ship identification numbers (Maritime Mobile Service Identity, or MMSI).– The NORAIS Receiver has a sample mode that can collect the raw signal, digitize it and send it to ground for analysis of signal quality, which is proving very helpful in making additional improvements/ refinements to the system. This is used both to investigate the signal environment and to evaluate the performance of new receiver technologies on the ground. Several hundred data sets have been collected and processed with new candidate algorithms for next generation receivers.– From the assessment of these data sets, an updated version of the decoder algorithm has been worked. The development benefits from the investigations of the sampled data and ongoing work in other ESA projects. The firmware was uploaded to the NORAIS Receiver through the station’s communications network. This upgrade #1 (“NORAIS Receiver FPGA firmware v18”), was activated on 1/20/2012.– The on-orbit data of the NORAIS Receiver v18 have been analyzed since and show very good results. The teams are confident in the operation and performance of v18 and have now preliminary results of the comparison of the performance of the upgraded NORAIS Receiver (v18) relative to the version operated prior to the upgrade (v16).– Changes of the signal environment on ISS can influence the number of correctly decoded messages, which makes it important to compare the results of this upgrade to a period running the old algorithm with a similar background level.– The daily averages are calculated for 11 days for both receiver versions. For the upgrade, the period considered for comparison is 1/21-1/31/2012, which are the first 11 days of operation. When selecting the period for the reference data it was important to find a period with the same background signal level as the 11 days with the upgraded NORAIS Receiver. The period from 11/27 – 12/7/2011 was. Even though the two 11 day periods are 45 days apart, the ship traffic should not be very different around the world, except for some regions in the north that may be hampered by sea ice.– The performance has been studied as the average number of decoded messages per day for the current upgrade v18 of the firmware and the original NORAIS Receiver software. The improvement is the ratio of these numbers (so average numbers of messages per day before the upgrade divided by number of messages after the upgrade). The number of messages from ships in various geographic areas shows a variation in the ratio of messages from 1.2 to 2.0, whereas the ratio of MMSI’s ranges from 1.1 to 1.9. The improvement in the Mediterranean is almost a factor of 2.0 in number of messages, and more than 1.6 in number of distinct ships per day. The improvement in other high-traffic zones, at the Gulf of Mexico and East Asia, is even higher.]

VESSEL IMAGING (ESA): “Thank you, Aki, for your first VESSEL IMAGING scan session. The science team reported very good scan images!” [Background: It is known that the ability of blood vessels to vasoconstrict – the ability of the muscular vessel wall to narrow the diameter of the blood vessel – is impaired during and after a human has been in space. “Vessel Imaging” is using the Ultrasound scanner on board the ISS to take images of the five different blood vessels in the lower abdomen and in the legs to study what changes occur to cause the blood vessels to be less able to vasoconstrict. For each vessel, a 5 second scan is performed to observe the blood vessel during several heart beats, followed by a scan where the ultrasound scan-head is tilted to allow a “cut through the blood vessel wall”. The same scans are also performed before flight, and these pre-flight images are used as the baseline to which the in-flight data is compared with. The images are analyzed to detect any changes in the blood vessel wall properties, such as wall thickness, elasticity or structure, changes in the size of the blood vessel or blood flow (volume) while the crewmember is in orbit.]

VIABLE (eValuatIon And monitoring of microBiofiLms insidE the ISS Payload Touch, NASA): “Thank you Suni for performing the touch activity this past Monday.”

VO2max (NASA): No report.

VLE (Video Lessons ESA): No report.

WAICO #1/#2 (Waving and Coiling of Arabidopsis Roots at Different g-levels; ESA): No report.

YEAST B (ESA): No report.

YOUTUBE SpaceLab: “Thanks so much for all of your work on the spiders. The close-up photos
of Nefertiti were excellent and we could even tell the gender of the fruit fly sitting next to the her! We appreciate it. We also really appreciate the pictures of her with the fruit-fly in her mouth from the feeding this morning. The red backed spider (Nefertiti) is doing really well. She is active and hunting ferociously. We have caught her jumping on video. We are not sure how she is managing it, but she is definitely jumping to catch flies. The Zebra spider (Cleopatra) is missing in action. We can tell by the webbing within the primary habitat that she came out of the water compartment and walked all around her habitat. She most likely did enter the fruit fly area behind the balsa wood via the fruit fly exit hole. This is disappointing, but not completely unexpected. We believe she is most likely still alive, but hiding and possibly eating within the fruit fly compartment.”

CEO (Crew Earth Observation): Through 7/21 the ground has received 1,748 of ISS CEO frames from Expedition 32 for review and cataloging. “We are pleased to report that we have received imagery with times corresponding to our CEO target request times as follows: Dodoma, Tanzania – 7 frames – 2 frames nearby, but target not acquired; and Mt. Kilimanjaro, Tanzania – 9 frames using 400mm lens – target acquired – best dry season imagery received in some time – we will continue to request this target with the 800mm lens. Thanks you for your efforts to acquire our targets. We are impressed with some of the imagery you are acquiring on your own time, particularly the nighttime imagery of cities, auroras, and even polar mesospheric clouds. These are features that we include in our target lists from time to time as conditions warrant. You look like you will be ready when we do! One of your very detailed images acquired at the time of the flooding event in the Krasnodar region of southern Russia was published on the Natural Hazards page of NASA/GSFC Earth Observatory website this past weekend. Your crisp, nicely composed 1200mm view of the city of Krymsk provided excellent context of the flood damaged area. Nice shot!”

WRM Update: A new WRM (Water Recovery Management) “cue card” was uplinked to the crew for their reference, updated with their latest CWC (Contingency Water Container) water audit. [The new card (32-0027D) lists 13 CWCs (218.8 L total) for the five types of water identified on board: 1. Silver technical water (4 CWCs with 149 3, plus 1 empty bag); 2. Condensate water (3 CWCs with 14.0 L, plus 2 empty bags); 3. Iodinated water (3 CWCs with 55.5 L); and 4. Waste water (1 empty bag EMU waste water). Also one leaky CWC (#1024) with 8.5 L). No bags with Wautersia bacteria. Other CWCs are stowed behind racks and are currently not being tracked due to unchanging contents. Wautersia bacteria are typical water-borne microorganisms that have been seen previously in ISS water sources. These isolates pose no threat to human health.]

Significant Events Ahead (all dates Eastern Time and subject to change):
————–Six-crew operations—————-
08/16/12 — Russian EVA-31
08/30/12 — US EVA-18
09/06/12 — HTV3 undocking
09/08/12 — HTV3 reentry
09/17/12 — Soyuz TMA-04M/30S undock/landing (End of Increment 32)
————–Three-crew operations————-
09/25/12 — ATV3 undocking
10/15/12 — Soyuz TMA-06M/32S launch – K.Ford (CDR-34)/O.Novitsky/E.Tarelkin
10/17/12 — Soyuz TMA-06M/32S docking
————–Six-crew operations————-
11/01/12 — Progress M-17M/49P launch
11/03/12 — Progress M-17M/49P docking
11/12/12 — Soyuz TMA-05M/31S undock/landing (End of Increment 33)
————–Three-crew operations————-
12/05/12 — Soyuz TMA-07M/33S launch – C.Hadfield (CDR-35)/T.Mashburn/R.Romanenko
12/07/12 — Soyuz TMA-07M/33S docking
————–Six-crew operations————-
12/26/12 — Progress M-18M/50P launch
12/28/12 — Progress M-18M/50P docking
03/19/13 — Soyuz TMA-06M/32S undock/landing (End of Increment 34)
————–Three-crew operations————-
04/02/13 — Soyuz TMA-08M/34S launch – P.Vinogradov (CDR-36)/C.Cassidy/A.Misurkin
04/04/13 — Soyuz TMA-08M/34S docking
————–Six-crew operations————-
05/16/13 — Soyuz TMA-07M/33S undock/landing (End of Increment 35)
————–Three-crew operations————-
05/29/13 — Soyuz TMA-09M/35S launch – M.Suraev (CDR-37)/K.Nyberg/L.Parmitano
05/31/13 — Soyuz TMA-09M/35S docking
————–Six-crew operations————-
09/xx/13 — Soyuz TMA-08M/34S undock/landing (End of Increment 36)
————–Three-crew operations————-
09/xx/13 — Soyuz TMA-10M/36S launch – M.Hopkins/TBD (CDR-38)/TBD
09/xx/13 — Soyuz TMA-10M/36S docking
————–Six-crew operations————-
11/xx/13 — Soyuz TMA-09M/35S undock/landing (End of Increment 37)
————–Three-crew operations————-
11/xx/13 — Soyuz TMA-11M/37S launch – K.Wakata (CDR-39)/R.Mastracchio/TBD
11/xx/13 — Soyuz TMA-11M/37S docking
————–Six-crew operations————-
03/xx/14 — Soyuz TMA-10M/36S undock/landing (End of Increment 38)
————–Three-crew operations————-

SpaceRef staff editor.