Commit e649e63e629584e87c69eb0e50bce1c5a9bc4a0d
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added comment on GEOTAIL when to use CPI and LEP
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NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl-cpi-swa.xml
... | ... | @@ -15,7 +15,13 @@ |
15 | 15 | the previously used 32 steps per spectrum. The change was made to ensure that |
16 | 16 | even for very cold flows, the spectrum would have a sufficient number of |
17 | 17 | significant points to derive moments. The change resulted in 96s spectra and |
18 | - 96s-resolution moments, vs. 48s previously. | |
18 | + 96s-resolution moments, vs. 48s previously. | |
19 | + CPI/SWEA and LEP measurement are expected to be used in a complementary way. LEP is highly sensitive and is dedicated to | |
20 | + measure tenuous plasma of the magnetosphere. However, when GEOTAIL is in the interplanetary, LEP generally scans only the | |
21 | + high energy (> 5 KeV) part of the ion distribution. This automated mode allows to assure long term preservation of the LEP | |
22 | + detectors. The LEP ion moments obtained in the inteerplanetary medium should be used only for qualitative purposes. | |
23 | + The ion moments in the interplanetary medium are provided by the CPI/SWEA instrument designed for | |
24 | + measuring the denser magnetosheath and solar wind plasma. | |
19 | 25 | </Description> |
20 | 26 | <Acknowledgement>In any publications, the use of the Geotail data should be acknowledged</Acknowledgement> |
21 | 27 | <Contact> | ... | ... |
NumericalData/CDPP-AMDA/GEOTAIL/LEP/gtl-lep-edb.xml
... | ... | @@ -12,7 +12,13 @@ |
12 | 12 | |
13 | 13 | The ion energy analyzer (LEP-EAi) has two energy scan mode: RAM-A (60 eV to 40 keV) and RAM-B (5 keV to 40 keV). RAM-B is selected to protect the very sensitive detector from intense low energy fluxes that are usually seen in the solar wind and magnetosheath. The energy scan mode is automatically selected onboard depending on incoming ion fluxes. At present, only the ion moments in the RAM-A mode are listed for the LEP-EAi data. |
14 | 14 | |
15 | - The ion moment data of the solar wind analyzer (LEP-SW) should be used only qualitatively. The LEP-SW ion moments are listed when the energy scan mode of LEP-EAi is RAM-B.</Description> | |
15 | + The ion moment data of the solar wind analyzer (LEP-SW) should be used only qualitatively. The LEP-SW ion moments are listed when the energy scan mode of LEP-EAi is RAM-B. | |
16 | + CPI/SWEA and LEP measurement are expected to be used in a complementary way. LEP is highly sensitive and is dedicated to measure | |
17 | + tenuous plasma of the magnetosphere. However, when GEOTAIL is in the interplanetary, LEP generally scans only the high energy | |
18 | + (> 5 KeV) part of the ion distribution. This automated mode allows to assure long term preservation of the LEP detectors. | |
19 | + The LEP ion moments obtained in the inteerplanetary medium should be used only for qualitative purposes. | |
20 | + The ion moments in the interplanetary medium are provided by the CPI/SWEA instrument designed for measuring the denser | |
21 | + magnetosheath and solar wind plasma.</Description> | |
16 | 22 | <Acknowledgement>In any publications, the use of the Geotail data should be acknowledged, for example, as "Geotail magnetic field data were provided by Y. Saito, JAXA in Japan."</Acknowledgement> |
17 | 23 | <Contact> |
18 | 24 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
Observatory/CDPP-AMDA/Geotail.xml
... | ... | @@ -11,7 +11,13 @@ |
11 | 11 | <AlternateName>ISTP/Geotail</AlternateName> |
12 | 12 | <AlternateName>GGS/Geotail</AlternateName> |
13 | 13 | <ReleaseDate>2016-08-05T18:19:18Z</ReleaseDate> |
14 | - <Description>The GEOTAIL mission is a collaborative project undertaken by the Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), and the National Aeronautics and Space Administration (NASA). The Geotail spacecraft was designed and built by ISAS and was launched on July 24, 1992. After fulfilling Its original objective of studying the dynamics of the Earth's magnetotail over a wide range of distance, extending from the near-Earth region (8 Earth radii (Re) from the Earth) to the distant tail (about 200 Re) its orbit was changed. Since February 1995 Geotail has been in an elliptical 9 by 30 Re orbit where it has provided data on most aspects of the solar wind interaction with the magnetosphere. | |
14 | + <Description>The GEOTAIL mission is a collaborative project undertaken by the Institute of Space and Astronautical Science (ISAS), | |
15 | + Japan Aerospace Exploration Agency (JAXA), and the National Aeronautics and Space Administration (NASA). | |
16 | + The Geotail spacecraft was designed and built by ISAS and was launched on July 24, 1992. | |
17 | + After fulfilling Its original objective of studying the dynamics of the Earth's magnetotail over a wide range of distance, | |
18 | + extending from the near-Earth region (8 Earth radii (Re) from the Earth) to the distant tail (about 200 Re) its orbit was changed. | |
19 | + Since February 1995 Geotail has been in an elliptical 9 by 30 Re orbit where it has provided data on most aspects of the solar wind | |
20 | + interaction with the magnetosphere. | |
15 | 21 | </Description> |
16 | 22 | <Contact> |
17 | 23 | <PersonID>spase://SMWG/Person/Guan.Le</PersonID> | ... | ... |