Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Galand, M. F."'
Autor:
Matteini, L., Horbury, T. S., Woodham, L. D., Bale, S. D., Hellinger, P., Galand, M. F., Jones, G. H., O'Brien, H., Evans, V., Angelini, V., Maksimovic, M., Chust, Thomas, Khotyaintsev, Y., Krasnoselskikh, V., Kretzschmar, Matthieu, Lorfevre, E., Plettemeier, D., Soucek, J., Steller, M., Stverak, S., Travnicek, P., Vaivads, A., Vecchio, A., Bruno, R., Fedorov, A., Livi, S. A., Louarn, P., Owen, C. J.
Comet ATLAS disintegrated into several fragments while reaching its most recent perihelion at approximately 0.25AU in April 2020. Solar Orbiter is predicted to have crossed both the ion and dust tails of the comet between 31 May and 6 June 2020, when
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______166::abc5c06950524a9ca8d21c18f4f6cf67
https://hal-insu.archives-ouvertes.fr/insu-03560093
https://hal-insu.archives-ouvertes.fr/insu-03560093
Autor:
Myllys, M. E., Pierre Henri, Goldstein, R., Galand, M. F., Gilet, N., Heritier, K. L., Burch, J. L.
Publikováno v:
HAL
A dynamic plasma environment is created around the comet when its expanding atmosphere gets ionized by solar EUV radiation and electron-impact ionization. The characteristics of the near-cometary plasma vary with the cometary activity phase (i.e., he
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::77fe7f90634ec3bcf7d638139224a14d
https://hal-insu.archives-ouvertes.fr/insu-03565550
https://hal-insu.archives-ouvertes.fr/insu-03565550
Autor:
Goetz, C., Tsurutani, B., Pierre Henri, Edberg, N. J. T., Volwerk, M., Nilsson, H., Mokashi, P., Heritier, K. L., Behar, E., Carr, C., Eriksson, A., Galand, M. F., Odelstad, E., Richter, I., Rubin, M., Simon Wedlund, C., Wellbrock, A., Glassmeier, K. H.
Publikováno v:
HAL
The magnetometer onboard ESA's Rosetta orbiter detected its highest magnetic field magnitude of 250nT in July 2015, close to perihelion. This magnitude was an enhancement of a factor of five compared to normal values, which makes this the highest int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::8498c33101603d60ade769e58f300128
https://hal-insu.archives-ouvertes.fr/insu-03570125
https://hal-insu.archives-ouvertes.fr/insu-03570125
Autor:
Hajra, R., Bruce, T., Pierre, H., Galand, M. F., Heritier, K. L., Edberg, N. J. T., Burch, J. L., Broiles, T. W., Goldstein, R., Glassmeier, K. H., Richter, I., Goetz, C., Nilsson, H., Altwegg, K., Rubin, M., Tanimori, T.
Cometary outbursts are one of the most spectacular aspects of comet behavior. They are characterized by an abrupt increase in cometary brightness followed by a gradual fall off to the pre-event brightness. Although there are several studies on outbur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______166::b1c9f79fb2c6acf5ac78b76dfa29089d
https://hal-insu.archives-ouvertes.fr/insu-03573490
https://hal-insu.archives-ouvertes.fr/insu-03573490
Autor:
Pierre Henri, Xavier Vallières, Gilet, N., Hajra, R., Moré, J., Goetz, C., Richter, I., Glassmeier, K. H., Galand, M. F., Heritier, K. L., Eriksson, A. I., Nemeth, Z., Tsurutani, B., Rubin, M., Altwegg, K.
Publikováno v:
HAL
At distances close enough to the Sun, when comets are characterised by a significant outgassing, the cometary neutral density may become large enough for both the cometary plasma and the cometary gas to be coupled, through ion-neutral and electron-ne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::60091d03d3c7420edc40854902dcb766
https://hal-insu.archives-ouvertes.fr/insu-03573488
https://hal-insu.archives-ouvertes.fr/insu-03573488