Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images
Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are consider...
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| Autor*in: |
Zasova, L. V. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2006 |
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| Anmerkung: |
© Pleiades Publishing, Inc. 2006 |
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| Übergeordnetes Werk: |
Enthalten in: Cosmic research - Nauka/Interperiodica, 1964, 44(2006), 4 vom: Juli, Seite 305-316 |
|---|---|
| Übergeordnetes Werk: |
volume:44 ; year:2006 ; number:4 ; month:07 ; pages:305-316 |
| Links: |
|---|
| DOI / URN: |
10.1134/S0010952506040046 |
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OLC2027382305 |
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| 245 | 1 | 0 | |a Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images |
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| 520 | |a Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. | ||
| 700 | 1 | |a Formisano, V. |4 aut | |
| 700 | 1 | |a Moroz, V. I. |4 aut | |
| 700 | 1 | |a Bibring, J. -P. |4 aut | |
| 700 | 1 | |a Grassi, D. |4 aut | |
| 700 | 1 | |a Ignatiev, N. I. |4 aut | |
| 700 | 1 | |a Giuranna, M. |4 aut | |
| 700 | 1 | |a Bellucci, G. |4 aut | |
| 700 | 1 | |a Altieri, F. |4 aut | |
| 700 | 1 | |a Blecka, M. |4 aut | |
| 700 | 1 | |a Gnedykh, V. N. |4 aut | |
| 700 | 1 | |a Grigoriev, A. V. |4 aut | |
| 700 | 1 | |a Lellouch, E. |4 aut | |
| 700 | 1 | |a Mattana, A. |4 aut | |
| 700 | 1 | |a Maturilli, A. |4 aut | |
| 700 | 1 | |a Moshkin, B. E. |4 aut | |
| 700 | 1 | |a Nikolsky, Yu. V. |4 aut | |
| 700 | 1 | |a Patsaev, D. V. |4 aut | |
| 700 | 1 | |a Piccioni, G. |4 aut | |
| 700 | 1 | |a Ratai, M. |4 aut | |
| 700 | 1 | |a Saggin, B. |4 aut | |
| 700 | 1 | |a Fonti, S. |4 aut | |
| 700 | 1 | |a Khatuntsev, I. V. |4 aut | |
| 700 | 1 | |a Hirsh, H. |4 aut | |
| 700 | 1 | |a Ekonomov, A. P. |4 aut | |
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10.1134/S0010952506040046 doi (DE-627)OLC2027382305 (DE-He213)S0010952506040046-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Zasova, L. V. verfasserin aut Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2006 Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. Formisano, V. aut Moroz, V. I. aut Bibring, J. -P. aut Grassi, D. aut Ignatiev, N. I. aut Giuranna, M. aut Bellucci, G. aut Altieri, F. aut Blecka, M. aut Gnedykh, V. N. aut Grigoriev, A. V. aut Lellouch, E. aut Mattana, A. aut Maturilli, A. aut Moshkin, B. E. aut Nikolsky, Yu. V. aut Patsaev, D. V. aut Piccioni, G. aut Ratai, M. aut Saggin, B. aut Fonti, S. aut Khatuntsev, I. V. aut Hirsh, H. aut Ekonomov, A. P. aut Enthalten in Cosmic research Nauka/Interperiodica, 1964 44(2006), 4 vom: Juli, Seite 305-316 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:44 year:2006 number:4 month:07 pages:305-316 https://doi.org/10.1134/S0010952506040046 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 44 2006 4 07 305-316 |
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10.1134/S0010952506040046 doi (DE-627)OLC2027382305 (DE-He213)S0010952506040046-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Zasova, L. V. verfasserin aut Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2006 Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. Formisano, V. aut Moroz, V. I. aut Bibring, J. -P. aut Grassi, D. aut Ignatiev, N. I. aut Giuranna, M. aut Bellucci, G. aut Altieri, F. aut Blecka, M. aut Gnedykh, V. N. aut Grigoriev, A. V. aut Lellouch, E. aut Mattana, A. aut Maturilli, A. aut Moshkin, B. E. aut Nikolsky, Yu. V. aut Patsaev, D. V. aut Piccioni, G. aut Ratai, M. aut Saggin, B. aut Fonti, S. aut Khatuntsev, I. V. aut Hirsh, H. aut Ekonomov, A. P. aut Enthalten in Cosmic research Nauka/Interperiodica, 1964 44(2006), 4 vom: Juli, Seite 305-316 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:44 year:2006 number:4 month:07 pages:305-316 https://doi.org/10.1134/S0010952506040046 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 44 2006 4 07 305-316 |
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10.1134/S0010952506040046 doi (DE-627)OLC2027382305 (DE-He213)S0010952506040046-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Zasova, L. V. verfasserin aut Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2006 Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. Formisano, V. aut Moroz, V. I. aut Bibring, J. -P. aut Grassi, D. aut Ignatiev, N. I. aut Giuranna, M. aut Bellucci, G. aut Altieri, F. aut Blecka, M. aut Gnedykh, V. N. aut Grigoriev, A. V. aut Lellouch, E. aut Mattana, A. aut Maturilli, A. aut Moshkin, B. E. aut Nikolsky, Yu. V. aut Patsaev, D. V. aut Piccioni, G. aut Ratai, M. aut Saggin, B. aut Fonti, S. aut Khatuntsev, I. V. aut Hirsh, H. aut Ekonomov, A. P. aut Enthalten in Cosmic research Nauka/Interperiodica, 1964 44(2006), 4 vom: Juli, Seite 305-316 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:44 year:2006 number:4 month:07 pages:305-316 https://doi.org/10.1134/S0010952506040046 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 44 2006 4 07 305-316 |
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10.1134/S0010952506040046 doi (DE-627)OLC2027382305 (DE-He213)S0010952506040046-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Zasova, L. V. verfasserin aut Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2006 Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. Formisano, V. aut Moroz, V. I. aut Bibring, J. -P. aut Grassi, D. aut Ignatiev, N. I. aut Giuranna, M. aut Bellucci, G. aut Altieri, F. aut Blecka, M. aut Gnedykh, V. N. aut Grigoriev, A. V. aut Lellouch, E. aut Mattana, A. aut Maturilli, A. aut Moshkin, B. E. aut Nikolsky, Yu. V. aut Patsaev, D. V. aut Piccioni, G. aut Ratai, M. aut Saggin, B. aut Fonti, S. aut Khatuntsev, I. V. aut Hirsh, H. aut Ekonomov, A. P. aut Enthalten in Cosmic research Nauka/Interperiodica, 1964 44(2006), 4 vom: Juli, Seite 305-316 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:44 year:2006 number:4 month:07 pages:305-316 https://doi.org/10.1134/S0010952506040046 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 44 2006 4 07 305-316 |
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10.1134/S0010952506040046 doi (DE-627)OLC2027382305 (DE-He213)S0010952506040046-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Zasova, L. V. verfasserin aut Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2006 Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. Formisano, V. aut Moroz, V. I. aut Bibring, J. -P. aut Grassi, D. aut Ignatiev, N. I. aut Giuranna, M. aut Bellucci, G. aut Altieri, F. aut Blecka, M. aut Gnedykh, V. N. aut Grigoriev, A. V. aut Lellouch, E. aut Mattana, A. aut Maturilli, A. aut Moshkin, B. E. aut Nikolsky, Yu. V. aut Patsaev, D. V. aut Piccioni, G. aut Ratai, M. aut Saggin, B. aut Fonti, S. aut Khatuntsev, I. V. aut Hirsh, H. aut Ekonomov, A. P. aut Enthalten in Cosmic research Nauka/Interperiodica, 1964 44(2006), 4 vom: Juli, Seite 305-316 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:44 year:2006 number:4 month:07 pages:305-316 https://doi.org/10.1134/S0010952506040046 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 44 2006 4 07 305-316 |
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Zasova, L. V. @@aut@@ Formisano, V. @@aut@@ Moroz, V. I. @@aut@@ Bibring, J. -P. @@aut@@ Grassi, D. @@aut@@ Ignatiev, N. I. @@aut@@ Giuranna, M. @@aut@@ Bellucci, G. @@aut@@ Altieri, F. @@aut@@ Blecka, M. @@aut@@ Gnedykh, V. N. @@aut@@ Grigoriev, A. V. @@aut@@ Lellouch, E. @@aut@@ Mattana, A. @@aut@@ Maturilli, A. @@aut@@ Moshkin, B. E. @@aut@@ Nikolsky, Yu. V. @@aut@@ Patsaev, D. V. @@aut@@ Piccioni, G. @@aut@@ Ratai, M. @@aut@@ Saggin, B. @@aut@@ Fonti, S. @@aut@@ Khatuntsev, I. V. @@aut@@ Hirsh, H. @@aut@@ Ekonomov, A. P. @@aut@@ |
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520 620 VZ 16,12 ssgn Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images |
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Zasova, L. V. Formisano, V. Moroz, V. I. Bibring, J. -P. Grassi, D. Ignatiev, N. I. Giuranna, M. Bellucci, G. Altieri, F. Blecka, M. Gnedykh, V. N. Grigoriev, A. V. Lellouch, E. Mattana, A. Maturilli, A. Moshkin, B. E. Nikolsky, Yu. V. Patsaev, D. V. Piccioni, G. Ratai, M. Saggin, B. Fonti, S. Khatuntsev, I. V. Hirsh, H. Ekonomov, A. P. |
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results of measurements with the planetary fourier spectrometer onboard mars express: clouds and dust at the end of southern summer. a comparison with omega images |
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Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images |
| abstract |
Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. © Pleiades Publishing, Inc. 2006 |
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Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. © Pleiades Publishing, Inc. 2006 |
| abstract_unstemmed |
Abstract We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Mars (Ls ∼ 340°). Three orbits are considered, two of which passed through volcanoes Olympus and Ascraeus Mons (the height above the surface is about +20 km), while the third orbit intersects lowland Hellas (−7 km). The influence of the relief on the properties of the aerosol observed is demonstrated: clouds of water ice with a visual optical thickness of 0.1–0.5 were observed above volcanoes, while only dust was found during the observations (close in time) along the orbit passing through Hellas in low and middle latitudes. This dust is homogeneously mixed with gas and has a reduced optical thickness of 0.25±0.05 (at v = 1100 $ cm^{−1} $). In addition to orographic clouds, ice clouds were observed in this season in the northern polar region. The clouds seen in the images obtained simultaneously by the mapping spectrometer OMEGA confirm the PFS results. Temperature inversion is discovered in the north polar hood below the level 1 mbar with a temperature maximum at about 0.6 mbar. This inversion is associated with descending movements in the Hadley cell. © Pleiades Publishing, Inc. 2006 |
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Results of measurements with the Planetary Fourier Spectrometer onboard Mars Express: Clouds and dust at the end of southern summer. A comparison with OMEGA images |
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