Google+ SpaceTravelFoundation: Radition effects
Showing posts with label Radition effects. Show all posts
Showing posts with label Radition effects. Show all posts

February 25, 2014

Be careful: Powerful X4.9-class solar flare recorded by SDO

Dear readers,

This night, a powerful X4.9-class solar flare has been recorded by NASA . This solar flare is the most intense flare of 2014 so far, and one of the most intense of the current solar cycle. Solar flare are really critical, specially for the spacecrafts orbiting Earth. Few weeks ago, the Orb-1 mission of the Antares rocket delayed due to high space radiation environment induced by a high class solar flare. Fortunately, the solar flare was not Earth directed.
The NASA's +SDO | Solar Dynamics Observatory recorded the extreme ultraviolet flash. After a solar flare during the next 3 days, all space partners are used to be very mindful in order to monitor the behavior of their spacecraft and anticipate some possible failures. Moreover, the ISS is used to be reoriented with the aim to protect its critical modules and the crew.



Stay tuned

January 8, 2014

Orb-1 mission of the Antares rocket delayed due to high space radiation environment

Dear followers,

yesterday, we announced that the Antares is already on the launch Pad-0A at +NASA's Wallops Flight Facility. This morning, the Antares launch team decided to delay the space launch due to an unusually high level of space radiation that exceeded by a considerable margin the constraints imposed on the mission to ensure the rocket's electronic systems are not impacted by a harsh radiation environment.

Image source : Orbital Science


The space rocket is in advance of a planned launch on January 8th at 1:32 p.m. EST on the Wallops Island, VA. The Orbital-1 mission is Orbital Sciences' first contracted cargo delivery flight to the space station for NASA. Among the cargo aboard Cygnus set to launch to the international space station are science experiments, crew provisions, and other hardware. 

Stay tuned 

[Update] : if the level of radiations moves down, Orbital Sciences announces that the launch could be performed on Thursday, the launch targeted launch time would be 1:10 p.m. (EST), with Cygnus arriving at the ISS Sunday morning, January 12.

April 12, 2013

MUSCA SEP3: A tool to assess the sensitivity of digital electronics in radiation environments such space


Space radiation environment is known to induce functional errors in electronics.
Particles, such as, neutrons, protons, or heavy ions, are known to induce these errors in electronics devices, so called SEE (Single Event Effects). These energetic particles can be induced by solar flares, comics rays, etc...
It’s critical for industrial and space agencies to evaluate this risk.
In this context, a new methodology of prediction is proposed in order to estimate the operational error rate for integrated devices boarded in space or avionic flights.


MUSCA SEP3 is a prediction tool for Single Event Effects (SEE), adapted to advanced digital technologies. 
It uses the Monte Carlo method, along with multi-scale and multi-physics modeling to estimate the sensitivity of a digital component in a given radiation environment. 

The MUSCA SEP3 predication tool is deployed by ONERA's Space Environment department (DESP), an acknowledged expert in modeling the radiation environment, and especially Single Event Effects (SEE). 
It is designed to assess and anticipate SEE risks, and provide technical and scientific support during the design hardening phases stipulated by the technology roadmap. 
Validations based on experimental data from accelerators and actual in-flight data have clearly demonstrated the performance of the MUSCA SEP3 tool in estimating SEE sensitivity on highly advanced components. 
The basic approach of the MUSCA SEP3 tool means that it can be easily used by manufacturers during the design phase. It simulates these effects by dividing the process into four very distinct stages, giving it a degree of flexibility adapted to SEE hardening.


The calibration of component models is based on ground test data or the results of TCAD simulations.
The description of the component design is based on the extraction of layout geometries from a GDS2 type file.
Physical simulation is based on a physical modeling of the digital component's transient electrical response.
Electrical simulation is carried out by injecting previously calculated transient currents into a circuit modeled under Spice, using the Cadence platform.


MUSCA SEP3 supports assessments for the space, atmospheric and terrestrial radiation environments. It can be used on all types of digital components calling on CMAS technology:
-          SRAM memories
-          Logic circuits and gates (NAND, XOR, MUX, etc.)
-          CMOS image sensors
-          Power PC.
The tool examines SEE sensitivity from an overall, very sophisticated perspective, to help all users (manufacturers, designers, end-users, etc.) meet their specific requirements:
-          Sensitivity mapping (heavy ions, neutrons, protons)
-          Calculating SEU/MCU/SET cross sections
-          Calculating operational SER
-          Aid in hardening design
General evaluation of a library of digital components.