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1by Määttänen, Anni, Lefèvre, Franck, Guilbon, Sabrina, Listowski, Constantino, Montmessin, Franck“... using SPICAM UV occultations. The UV channel measures spectra between 118 and 320 nm. The occultation...”
Published 2018
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2by Määttänen, Anni, Lefèvre, Franck, Guilbon, Sabrina, Listowski, Constantino, Montmessin, Franck“... using SPICAM UV occultations. The UV channel measures spectra between 118 and 320 nm. The occultation...”
Published 2018
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3by Määttänen, Anni, Lefèvre, Franck, Guilbon, Sabrina, Listowski, Constantino, Montmessin, Franck“... using SPICAM UV occultations. The UV channel measures spectra between 118 and 320 nm. The occultation...”
Published 2018
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4by Määttänen, Anni, Lefèvre, Franck, Guilbon, Sabrina, Listowski, Constantino, Montmessin, Franck“... using SPICAM UV occultations. The UV channel measures spectra between 118 and 320 nm. The occultation...”
Published 2018
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5by Määttänen, Anni, Lefèvre, Franck, Guilbon, Sabrina, Listowski, Constantino, Montmessin, Franck“... using SPICAM UV occultations. The UV channel measures spectra between 118 and 320 nm. The occultation...”
Published 2018
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6by Maltagliati, Luca, Fedorova, Anna, Montmessin, Franck, Bertaux, Jean-Loup, Korablev, Oleg, Reberac, Aurélie“... is mainly based on GCMs. The solar occultation dataset obtained by the SPICAM spectrometer on the Mars...”
Published 2010
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7by Maltagliati, Luca, Fedorova, Anna, Montmessin, Franck, Bertaux, Jean-Loup, Korablev, Oleg, Reberac, Aurélie“... is mainly based on GCMs. The solar occultation dataset obtained by the SPICAM spectrometer on the Mars...”
Published 2010
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8by Maltagliati, Luca, Fedorova, Anna, Montmessin, Franck, Bertaux, Jean-Loup, Korablev, Oleg, Reberac, Aurélie“... is mainly based on GCMs. The solar occultation dataset obtained by the SPICAM spectrometer on the Mars...”
Published 2010
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9by Maltagliati, Luca, Fedorova, Anna, Montmessin, Franck, Bertaux, Jean-Loup, Korablev, Oleg, Reberac, Aurélie“... is mainly based on GCMs. The solar occultation dataset obtained by the SPICAM spectrometer on the Mars...”
Published 2023
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10by Montmessin, Franck, Groeller, Hannes, Lacombe, Gaetan, Schneider, Nicholas M., Yelle, Roger, Stewart, Ian, Deighan, Justin, Clarke, John, Lefèvre, Franck, Baggio, Lucio, Mcclintock, William E., Holsclaw, Greg M., Jakosky, Bruce M.“... performing stellar occultations observations. In the IUVS wavelength range, CO2 possesses a distinct...”
Published 2015
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11by Montmessin, Franck, Groeller, Hannes, Lacombe, Gaetan, Schneider, Nicholas M., Yelle, Roger, Stewart, Ian, Deighan, Justin, Clarke, John, Lefèvre, Franck, Baggio, Lucio, Mcclintock, William E., Holsclaw, Greg M., Jakosky, Bruce M.“... performing stellar occultations observations. In the IUVS wavelength range, CO2 possesses a distinct...”
Published 2015
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12by Montmessin, Franck, Groeller, Hannes, Lacombe, Gaetan, Schneider, Nicholas M., Yelle, Roger, Stewart, Ian, Deighan, Justin, Clarke, John, Lefèvre, Franck, Baggio, Lucio, Mcclintock, William E., Holsclaw, Greg M., Jakosky, Bruce M.“... performing stellar occultations observations. In the IUVS wavelength range, CO2 possesses a distinct...”
Published 2015
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13by Montmessin, Franck, Groeller, Hannes, Lacombe, Gaetan, Schneider, Nicholas M., Yelle, Roger, Stewart, Ian, Deighan, Justin, Clarke, John, Lefèvre, Franck, Baggio, Lucio, Mcclintock, William E., Holsclaw, Greg M., Jakosky, Bruce M.“... performing stellar occultations observations. In the IUVS wavelength range, CO2 possesses a distinct...”
Published 2015
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14by Montmessin, Franck, Groeller, Hannes, Lacombe, Gaetan, Schneider, Nicholas M., Yelle, Roger, Stewart, Ian, Deighan, Justin, Clarke, John, Lefèvre, Franck, Baggio, Lucio, Mcclintock, William E., Holsclaw, Greg M., Jakosky, Bruce M.“... performing stellar occultations observations. In the IUVS wavelength range, CO2 possesses a distinct...”
Published 2015
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15by Montmessin, Franck, Groeller, Hannes, Lacombe, Gaetan, Schneider, Nicholas M., Yelle, Roger, Stewart, Ian, Deighan, Justin, Clarke, John, Lefèvre, Franck, Baggio, Lucio, Mcclintock, William E., Holsclaw, Greg M., Jakosky, Bruce M.“... performing stellar occultations observations. In the IUVS wavelength range, CO2 possesses a distinct...”
Published 2015
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16by Fedorova, A., Korablev, Oleg, Vandaele, A.-C., Bertaux, Jean-Loup, Belyaev, D., Mahieux, A., Neefs, E., Wilquet, W.V., Drummond, R., Montmessin, Franck, Villard, Eric“... and HDO in the Venus mesosphere have been obtained using Solar Occultation at Infrared (SOIR), a high...”
Published in Journal of Geophysical Research (2008)
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17by Fedorova, A., Korablev, Oleg, Vandaele, A.-C., Bertaux, Jean-Loup, Belyaev, D., Mahieux, A., Neefs, E., Wilquet, W.V., Drummond, R., Montmessin, Franck, Villard, Eric“... and HDO in the Venus mesosphere have been obtained using Solar Occultation at Infrared (SOIR), a high...”
Published in Journal of Geophysical Research (2008)
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18by Fedorova, A., Korablev, Oleg, Vandaele, A.-C., Bertaux, Jean-Loup, Belyaev, D., Mahieux, A., Neefs, E., Wilquet, W.V., Drummond, R., Montmessin, Franck, Villard, Eric“... and HDO in the Venus mesosphere have been obtained using Solar Occultation at Infrared (SOIR), a high...”
Published in Journal of Geophysical Research (2008)
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19by Fedorova, A., Korablev, Oleg, Vandaele, A.-C., Bertaux, Jean-Loup, Belyaev, D., Mahieux, A., Neefs, E., Wilquet, W.V., Drummond, R., Montmessin, Franck, Villard, Eric“... and HDO in the Venus mesosphere have been obtained using Solar Occultation at Infrared (SOIR), a high...”
Published in Journal of Geophysical Research (2008)
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20by Bertaux, Jean-Loup, Gagné, Marie-Eve, Montmessin, Franck, Gonzalez-Galindo, Francisco, Lefèvre, Franck“... occultations (more than 2000), which in about 10% cases revealed the presence of the NO emission in addition...”
Published 2013
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