Zobrazeno 1 - 10
of 55
pro vyhledávání: '"H. A. Zook"'
Autor:
H. A. Zook, Stanley F. Dermott, Bo Å. S. Gustafson, D. Linkert, Douglas P. Hamilton, G. Linkert, Mihaly Horanyi, J. A. M. McDonnell, D. Bindschadler, Gregor E. Morfill, Ingrid Mann, Richard Moissl, Eberhard Grün, Gerhard Schwehm, Martha S. Hanner, Ralf Srama, Bertil Anders Lindblad, Amara L. Graps, C. Polanskey, Harald Krüger, Jochen Kissel
Publikováno v:
Planetary and Space Science. 54:879-910
The dust detector system on board the Galileo spacecraft recorded dust impacts in circumjovian space during the craft's orbital mission about Jupiter. This is the eighth in a series of papers dedicated to presenting Galileo and Ulysses dust data. We
Autor:
Mihaly Horanyi, Markus Landgraf, D. Möhlmann, D. Linkert, Ralf Srama, Valeri Dikarev, H. A. Zook, Ove Havnes, M. Stübig, M. Görlich, Alexander V. Krivov, A. Mocker-Ahlreep, M. Müller, J. Svestka, G. Schlotzhauer, Nicolas Altobelli, Philippe Lamy, Thanasis E. Economou, J. G. Bradley, V. Tschernjawski, Georg Moragas-Klostermeyer, Thomas J. Ahrens, S. Helfert, Hugo Fechtig, Gerhard Schäfer, G. Linkert, Eberhard Grün, J. A. M. McDonnell, Anthony J. Tuzzolino, M. E. Burton, Frank Spahn, S. Auer, Harald Krüger, Eduard Igenbergs, Manuel Grande, Elmar K. Jessberger, Torrence V. Johnson, M. Roy, Amara L. Graps, Sascha Kempf, Gerhard Schwehm, F. Lura, Gregor E. Morfill, R. Wäsch
Publikováno v:
Space Science Reviews. 114:465-518
The Cassini-Huygens Cosmic Dust Analyzer (CDA) is intended to provide direct observations of dust grains with masses between 10-19 and 10-9 kg in interplanetary space and in the jovian and satumian systems, to investigate their physical, chemical and
Autor:
Stanley F. Dermott, Ralf Srama, Gregor E. Morfill, Amara L. Graps, Gerhard Schwehm, M. S. Hanner, Douglas P. Hamilton, Mihaly Horanyi, Ingrid Mann, H. A. Zook, D. Bindschadler, D. Linkert, Jochen Kissel, G. Linkert, Eberhard Grün, Hugo Fechtig, Bertil Anders Lindblad, H. Krüger, B. A. Gustason, C. Planskey, J. A. M. McDonnell
Publikováno v:
Planetary and Space Science. 49:1285-1301
The dust detector system onboard Galileo records dust impacts in circumjovian space since the spacecraft has been injected into a bound orbit about Jupiter in December 1995. This is the sixth in a series of papers dedicated to presenting Galileo and
Autor:
J. A. M. McDonnell, D. Linkert, Mihaly Horanyi, Eberhard Grün, Ingrid Mann, Markus Landgraf, Martha S. Hanner, Stanley F. Dermott, Bo Å. S. Gustafson, G. Linkert, M. Baguhl, H. Fechtig, Harald Krüger, Jochen Kissel, Douglas P. Hamilton, Ralf Srama, Gerhard Schwehm, H. A. Zook, Gregor E. Morfill, C. Polanskey, Bertil Anders Lindblad
Publikováno v:
Scopus-Elsevier
The Ulysses spacecraft is orbiting the Sun on a highly inclined ellipse (i = 79°). After its Jupiter flyby in 1992 at a heliocentric distance of 5.4 AU, the spacecraftreapproached the inner solar system, flew over the Suns south polar region in Sept
Autor:
H. Fechtig, Jochen Kissel, H. A. Zook, Mihaly Horanyi, G. Linkert, Ralf Srama, D. Linkert, P. Staubach, Martha S. Hanner, Bertil Anders Lindblad, C. Polanskey, Ingrid Mann, Gregor E. Morfill, Eberhard Grün, Gerhard Schwehm, Stanley F. Dermott, Bo Å. S. Gustafson, M. Baguhl, Douglas P. Hamilton, J. A. M. McDonnell
Publikováno v:
Icarus. 129:270-288
Identical in situ dust detectors are flown on board the Galileo and Ulysses spacecraft. They record impacts of micrometeoroids in the ecliptic plane at heliocentric distances from 0.7 to 5.4 AU and in a plane almost perpendicular to the ecliptic from
Autor:
Martha S. Hanner, C. Polanskey, Stanley F. Dermott, Bo Å. S. Gustafson, H. A. Zook, H. Fechtig, Douglas P. Hamilton, G. Linkert, A. Heck, Harald Krüger, Jochen Kissel, Eberhard Grün, Amara L. Graps, D. Linkert, Mihaly Horanyi, Ingrid Mann, J. A. M. McDonnell, Ralf Srama, Gerhard Schwehm, Gregor E. Morfill, Bertil Anders Lindblad
Publikováno v:
Scopus-Elsevier
Dust measurements have been obtained with the dust detector onboard the Galileo spacecraft inside a distance of about 60RJ from Jupiter (Jupiter radius, RJ = 71,492 km) during two periods of about 8 days around Galileo's closest approaches to Ganymed
Publikováno v:
International Astronomical Union Colloquium. 150:333-336
Over 700 photographs of the inner zodiacal light were taken from the Clementine spacecraft while it was in orbit around the Moon. These exposures were taken with the 28° x 43° field-of-view Star Tracker camera and the 4.2° x 5.6° field-of-view UV
Autor:
Bertil Anders Lindblad, N. Siddique, R. Riemann, Gerhard Schwehm, M. Baguhl, H. A. Zook, Douglas P. Hamilton, Gregor E. Morfill, Jochen Kissel, J. A. M. McDonnell, Ingrid Mann, Martha S. Hanner, G. Linkert, Hugo Fechtig, N. Divine, D. Linkert, Eberhard Grün, P. Staubach, C. Polanskey
Publikováno v:
Planetary and Space Science. 43:971-999
From October 18, 1990 to February 8, 1992 the Ulysses spacecraft traversed interplanetary space between the Earth and Jupiter; at Jupiter the spacecraft was deflected below the ecliptic onto a highly-inclined orbit ( i ∼80°). Here, we report on du
Autor:
D. Linkert, M. Baguhl, N. Divine, H. A. Zook, C. Polanskey, Douglas P. Hamilton, Eberhard Grün, R. Riemann, H. Fechtig, J. A. M. McDonnell, Gerhard Schwehm, P. Staubach, Gregor E. Morfill, Bertil Anders Lindblad, Ingrid Mann, Jochen Kissel, N. Siddique, G. Linkert, Martha S. Hanner
Publikováno v:
Planetary and Space Science. 43:953-969
From its launch in October 1989 until the end of 1992, the Galileo spacecraft traversed interplanetary space from Venus to the asteroid belt and successfully executed close flybys of Venus, the Earth, and the asteroid Gaspra. The dust instrument has
Autor:
Eberhard Grün, Stanley F. Dermott, Bertil Anders Lindblad, M. Baguhl, H. Fechtig, Jochen Kissel, Martha S. Hanner, Douglas P. Hamilton, P. Staubach, C. A. Polanskey, G. Linkert, R. Riemann, Gregor E. Morfill, H. A. Zook, D. Linkert, Mann, Gerhard Schwehm, J. A. M. McDonnell
Publikováno v:
Science. 268:1016-1019
Along Ulysses' path from Jupiter to the south ecliptic pole, the onboard dust detector measured a dust impact rate that varied slowly from 0.2 to 0.5 impacts per day. The dominant component of the dust flux arrived from an ecliptic latitude and longi