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Instrument/AMDA/Helios2/MAG.xml
| ... | ... | @@ -7,7 +7,7 @@ |
| 7 | 7 | <ResourceName>MAG</ResourceName> |
| 8 | 8 | <AlternateName>Helios Magnetometers : E2, E3</AlternateName> |
| 9 | 9 | <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate> |
| 10 | - <Description>>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to | |
| 10 | + <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to | |
| 11 | 11 | continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain |
| 12 | 12 | phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and |
| 13 | 13 | discontinuities. The measurement ranges are ± 100 nT and ± 400 nT. The resolution is ± 0.2 nT and ± |
| ... | ... | @@ -30,7 +30,6 @@ in the presence of discontinuities with magnetic field variations. |
| 30 | 30 | E3 : The Rome‐GSFC magnetic field experiment utilized a triaxial fluxgate (saturable inductor) |
| 31 | 31 | magnetometer. |
| 32 | 32 | </Description> |
| 33 | - <Contact> | |
| 34 | 33 | <Contact> |
| 35 | 34 | <PersonID>spase://CDPP/Person/Musmann</PersonID> |
| 36 | 35 | <Role>PrincipalInvestigator</Role> |
| ... | ... | @@ -39,6 +38,7 @@ magnetometer. |
| 39 | 38 | <PersonID>spase://CDPP/Person/Mariani</PersonID> |
| 40 | 39 | <Role>PrincipalInvestigator</Role> |
| 41 | 40 | </Contact> |
| 41 | + <Contact> | |
| 42 | 42 | <PersonID>spase://SMWG/Person/Norman.F.Ness</PersonID> |
| 43 | 43 | <Role>PrincipalInvestigator</Role> |
| 44 | 44 | </Contact> | ... | ... |