Difference between revisions of "Radiation environment"

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(Note: Adapted from Planck Collaboration 2011, A&A 536, A1)  
 
(Note: Adapted from Planck Collaboration 2011, A&A 536, A1)  
  
The Standard Radiation Environment Monitor on board Planck (SREM, Buehler et al. 1996) is a particle detector which is being flown on several ESA satellites. The SREM consists of several detectors sensitive to different energy ranges, which can also be used in coincidence mode. In particular, the SREM measures count rates of high energy protons (from  ~10 MeV to  ~300 MeV) and electrons (~300 keV to  ~6 MeV).
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The Standard Radiation Environment Monitor on board Planck (SREM, Buehler et al. 1996) is a particle detector which is being flown on several ESA satellites. The SREM consists of several detectors sensitive to different energy ranges, which can also be used in coincidence mode. In particular, the SREM measures count rates of high energy protons (from  ~20 MeV to  <math>\infty</math>) and electrons (~500 keV to  <math>\infty</math>).
  
 
Particle fluxes measured by the SREM on board Planck are shown in Fig. 8. The radiation environment of Planck is characterised by the current epoch near the minimum in the solar cycle. As a consequence, the particle flux is dominated by Galactic cosmic rays, rather than by the solar wind. The time evolution of the SREM measurements is well correlated with that of identical units flying simultaneously on other satellites (e.g., Herschel, Rosetta) and with indicators of Galactic cosmic rays, and is anti-correlated with solar flare events and with the solar cycle (Fig. 8). More importantly for Planck, the SREM measurements are very well correlated with the heat deposition on the coldest stages of the HFI, and with glitch rates measured by the detectors of HFI. A more detailed interpretation of these data is provided in Planck HFI Core Team (2011a).  
 
Particle fluxes measured by the SREM on board Planck are shown in Fig. 8. The radiation environment of Planck is characterised by the current epoch near the minimum in the solar cycle. As a consequence, the particle flux is dominated by Galactic cosmic rays, rather than by the solar wind. The time evolution of the SREM measurements is well correlated with that of identical units flying simultaneously on other satellites (e.g., Herschel, Rosetta) and with indicators of Galactic cosmic rays, and is anti-correlated with solar flare events and with the solar cycle (Fig. 8). More importantly for Planck, the SREM measurements are very well correlated with the heat deposition on the coldest stages of the HFI, and with glitch rates measured by the detectors of HFI. A more detailed interpretation of these data is provided in Planck HFI Core Team (2011a).  
  
(Adapted From the Herschel Observers manual)
 
The L2 environment (and orbits around it) is relatively benign compared to those in geostationary (GO), or low Earth (LEO) orbits. In particular, a series of common threats for satellites in GO or LEO, including the neutral thermosphere, space debris, geomagnetically trapped particles and large temperature gradients, are not a concern for L2 orbits. Environmental aspects to be considered at L2 include:
 
 
#Solar wind plasma. Essentially a neutral or cold plasma: 95% protons, 5% He++ and equivalent electrons; 1-10 particles/cm3. The main risk associated is a low surface charging potential. This plasma may be relatively benign at L2 compared to that found at GO and LEO.
 
 
#Ionising radiation: solar flares (energetic electrons, protons and alpha particles), Galactic cosmic rays and Jovian electrons.
 
 
#Magnetic fields: Earth's magnetotail extends up to 1000 Earth's radii, so it must be considered (2-10 nT) along with interplanetary magnetic field (∼ 5 nT). The effects on the spacecraft and PLM include possible orbit disturbance and electrostatic discharge (ESD).
 
 
Therefore, the main radiation components at L2 consist of: Galactic cosmic rays, solar particle events and solar and Jovian electrons.
 
 
In the early stages of the mission, the dominant radiation source was Jovian electrons, characterised by a energetic population and a 13-month synodic year modulation.
 
 
The Herschel spacecraft is equipped with a standard radiation environment monitor (SREM) placed in the -Z SVM panel; the SREM is a particle detector developed for satellite applications that has been added to Herschel and Planck as a passenger. It measures high-energy electrons (from 0.5 MeV to infinity) and protons (from 20 MeV to infinity) of the space environment with an angular resolution of some 20 degrees, providing particle species and spectral information. The SREM data are received on-ground and processed by the Space Weather Group at ESTEC, providing valuable information on the radiation environment at L2. A sample plot showing the calibrated count rates in three counters (TC1 - protons with E > 20 MeV; TC2 - protons with E > 39 MeV; TC3 - electrons with E > 0.5 MeV) is displayed in Figure 4.3 .
 
  
 
[[Category:Ground Segment and Operations]]
 
[[Category:Ground Segment and Operations]]

Revision as of 09:28, 28 August 2012

(Note: Adapted from Planck Collaboration 2011, A&A 536, A1)

The Standard Radiation Environment Monitor on board Planck (SREM, Buehler et al. 1996) is a particle detector which is being flown on several ESA satellites. The SREM consists of several detectors sensitive to different energy ranges, which can also be used in coincidence mode. In particular, the SREM measures count rates of high energy protons (from ~20 MeV to [math]\infty[/math]) and electrons (~500 keV to [math]\infty[/math]).

Particle fluxes measured by the SREM on board Planck are shown in Fig. 8. The radiation environment of Planck is characterised by the current epoch near the minimum in the solar cycle. As a consequence, the particle flux is dominated by Galactic cosmic rays, rather than by the solar wind. The time evolution of the SREM measurements is well correlated with that of identical units flying simultaneously on other satellites (e.g., Herschel, Rosetta) and with indicators of Galactic cosmic rays, and is anti-correlated with solar flare events and with the solar cycle (Fig. 8). More importantly for Planck, the SREM measurements are very well correlated with the heat deposition on the coldest stages of the HFI, and with glitch rates measured by the detectors of HFI. A more detailed interpretation of these data is provided in Planck HFI Core Team (2011a).

Space Radiation Environment Monitor

European Space Agency

(Planck) High Frequency Instrument