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Intensities of the Venusian N2 electron-impact excited dayglow emissions
DOI: 10.1002/2013JA019277 Bibcode: 2013JGRA..118.7850F

Fox, Jane L.; F. Hać, Nicholas E.

Dayglow emissions are signatures of both the energy deposition into an atmosphere and the abundances of the species from which they arise. The first N2 dayglow emissions from Mars, the (0,5) and (0,6) bands of the N2 Vegard-Kaplan band system, were detected by the Spectroscopy for Investigations of the Characteristics of the …

2013 Journal of Geophysical Research (Space Physics)
VenusExpress 2
Correction to "Variation of the Martian ionospheric electron density from Mars Express radar soundings"
DOI: 10.1002/jgra.50369 Bibcode: 2013JGRA..118.4710M

Gurnett, D. A.; Morgan, D. D.; Plaut, J. J. +3 more

2013 Journal of Geophysical Research (Space Physics)
MEx 2
Magnetic field topology of the plasma sheet boundary layer
DOI: 10.1002/jgra.50435 Bibcode: 2013JGRA..118.4059T

Nakamura, R.; Baumjohann, W.; Teh, W. -L.

magnetic field topology of the plasma sheet boundary layer (PSBL) and its neighborhood is examined using a steady, two-dimensional (2-D), ideal MHD reconstruction method. We study four PSBL crossings, from the lobe toward the plasma sheet and back into the lobe, by the Cluster spacecraft in the Earth's magnetotail around (x, y, z) = (-17.3, 4.3, -…

2013 Journal of Geophysical Research (Space Physics)
Cluster 1
Ulysses observations of Jupiter's 10 h modulation in interplanetary space in 2004
DOI: 10.1002/jgra.50430 Bibcode: 2013JGRA..118.4021D

Heber, B.; Kopp, A.; Dunzlaff, P.

Since the Pioneer 10/11 mission, Jupiter is known as a dominant and almost constant source of MeV electrons in the inner heliosphere. An interesting feature of the Jovian electron source is the fact that Jupiter's rotation period (~10 h) can frequently be recovered in the energy spectrum of Jovian electrons in the vicinity of the planet. However, …

2013 Journal of Geophysical Research (Space Physics)
Ulysses 0