Search

Your search keyword '"Ignatiev, N."' showing total 267 results
Start Over Author "Ignatiev, N."
267 results on '"Ignatiev, N."'

1. Unambiguous detection of mesospheric CO2 clouds on Mars using 2.7 {\mu}m absorption band from the ACS/TGO solar occultations

Author

Luginin, M., Trokhimovskiy, A., Fedorova, A., Belyaev, D., Ignatiev, N., Korablev, O., Montmessin, F., and Grigoriev, A.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

Mesospheric CO2 clouds are one of two types of carbon dioxide clouds known on Mars. We present observations of mesospheric CO2 clouds made by Atmospheric Chemistry Suit (ACS) onboard the ESA-Roscosmos ExoMars Trace Gas Orbiter (TGO). We analyzed 1663 solar occultation sessions of Thermal InfraRed (TIRVIM) and Middle InfraRed (MIR) channels of ACS covering more than two Martian years that contain spectra of 2.7 {\mu}m carbon dioxide ice absorption band. That allowed us to unambiguously discriminate carbon dioxide ice aerosols from mineral dust and water ice aerosols, not relying on the information of atmospheric thermal conditions. CO2 clouds were detected in eleven solar occultation observations at altitudes from 39 km to 90 km. In five cases, there were two or three layers of CO2 clouds that were vertically separated by 5-15 km gaps. Effective radius of CO2 aerosol particles is in the range of 0.1-2.2 {\mu}m. Spectra produced by the smallest particles indicate a need for a better resolved CO2 ice refractive index. Nadir optical depth of CO2 clouds is in the range 5*10^{-4}-4*10^{-2} at both 2.7 {\mu}m and 0.8 {\mu}m. Asymmetrical diurnal distribution of detections observed by ACS is potentially due to local time variations of temperature induced by thermal tides. Two out of five cases of carbon dioxide cloud detections made by the TIRVIM instrument reveal the simultaneous presence of CO2 ice and H2O ice aerosols. Temperature profiles measured by the Near InfraRed (NIR) channel of ACS are used to calculate CO2 saturation ratio S at locations of carbon dioxide clouds. Supersaturation S > 1 is detected in only 5 out of 19 cases of CO2 cloud layers; extremely low values of S < 0.1 are found in 9 out of 19 cases., Comment: 29 pages, 10 figures. Submitted to Icarus

Published
2024
Full Text
View/download PDF

3. Thermal structure and aerosols in Mars' atmosphere from TIRVIM/ACS onboard the ExoMars Trace Gas Orbiter : validation of the retrieval algorithm

Author

Guerlet, Sandrine, Ignatiev, N., Forget, F., Fouchet, T., Vlasov, P., Bergeron, G., Young, R. M. B., Millour, E., Fan, S., Tran, H., Shakun, A., Grigoriev, A., Trokhimovskiy, A., Montmessin, F., and Korablev, O.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

The Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter (TGO) monitors the Martian atmosphere through different spectral intervals in the infrared light. We present a retrieval algorithm tailored to the analysis of spectra acquired in nadir geometry by TIRVIM, the thermal infrared channel of ACS. Our algorithm simultaneously retrieves vertical profile of atmospheric temperature up to 50 km, surface temperature, and integrated optical depth of dust and water ice clouds. The specificity of the TIRVIM dataset lies in its capacity to resolve the diurnal cycle over a 54 sol period. However, it is uncertain to what extent can the desired atmospheric quantities be accurately estimated at different times of day. Here we first present an Observing System Simulation Experiment (OSSE). We produce synthetic observations at various latitudes, seasons and local times and run our retrieval algorithm on these synthetic data, to evaluate its robustness. Different sources of biases are documented, in particular regarding aerosol retrievals. Atmospheric temperature retrievals are found robust even when dust and/or water ice cloud opacities are not well estimated in our OSSE. We then apply our algorithm to TIRVIM observations in April-May, 2018 and perform a cross-validation of retrieved atmospheric temperature and dust integrated opacity by comparisons with thousands of co-located Mars Climate Sounder (MCS) retrievals. Most differences between TIRVIM and MCS atmospheric temperatures can be attributed to differences in vertical sensitivity. Daytime dust opacities agree well with each other, while biases are found in nighttime dust opacity retrieved from TIRVIM at this season., Comment: 51 pages, 29 figures. Accepted in Juanuary 2022 for publication in Journal of Geophysical Research (Planets)

Published
2022
Full Text
View/download PDF

4. Moons and Jupiter Imaging Spectrometer (MAJIS) on Jupiter Icy Moons Explorer (JUICE)

Author

Poulet, F., Piccioni, G., Langevin, Y., Dumesnil, C., Tommasi, L., Carlier, V., Filacchione, G., Amoroso, M., Arondel, A., D’Aversa, E., Barbis, A., Bini, A., Bolsée, D., Bousquet, P., Caprini, C., Carter, J., Dubois, J.-P., Condamin, M., Couturier, S., Dassas, K., Dexet, M., Fletcher, L., Grassi, D., Guerri, I., Haffoud, P., Larigauderie, C., Le Du, M., Mugnuolo, R., Pilato, G., Rossi, M., Stefani, S., Tosi, F., Vincendon, M., Zambelli, M., Arnold, G., Bibring, J.-P., Biondi, D., Boccaccini, A., Brunetto, R., Carapelle, A., Cisneros González, M., Hannou, C., Karatekin, O., Le Cle’ch, J.-C., Leyrat, C., Migliorini, A., Nathues, A., Rodriguez, S., Saggin, B., Sanchez-Lavega, A., Schmitt, B., Seignovert, B., Sordini, R., Stephan, K., Tobie, G., Zambon, F., Adriani, A., Altieri, F., Bockelée, D., Capaccioni, F., De Angelis, S., De Sanctis, M.-C., Drossart, P., Fouchet, T., Gérard, J.-C., Grodent, D., Ignatiev, N., Irwin, P., Ligier, N., Manaud, N., Mangold, N., Mura, A., Pilorget, C., Quirico, E., Renotte, E., Strazzulla, G., Turrini, D., Vandaele, A.-C., Carli, C., Ciarniello, M., Guerlet, S., Lellouch, E., Mancarella, F., Morbidelli, A., Le Mouélic, S., Raponi, A., Sindoni, G., and Snels, M.

Published
2024
Full Text
View/download PDF

11. Science objectives and performances of NOMAD, a spectrometer suite for the ExoMars TGO mission

Author

Vandaele, A.C., Neefs, E., Drummond, R., Thomas, I.R., Daerden, F., Lopez-Moreno, J.-J., Rodriguez, J., Patel, M.R., Bellucci, G., Allen, M., Altieri, F., Bolsée, D., Clancy, T., Delanoye, S., Depiesse, C., Cloutis, E., Fedorova, A., Formisano, V., Funke, B., Fussen, D., Geminale, A., Gérard, J.-C., Giuranna, M., Ignatiev, N., Kaminski, J., Karatekin, O., Lefèvre, F., López-Puertas, M., López-Valverde, M., Mahieux, A., McConnell, J., Mumma, M., Neary, L., Renotte, E., Ristic, B., Robert, S., Smith, M., Trokhimovsky, S., Vander Auwera, J., Villanueva, G., Whiteway, J., Wilquet, V., and Wolff, M.

Published
2015
Full Text
View/download PDF

13. Venera-D Mission Concept to Study Atmosphere, Surface and Plasma Environment: Phase II Report of the Venera-D Joint Science Definition Team

Author

Zasova, L, Gregg, T, Burdanov, A, Economou, T, Eismont, N, Gerasimov, M, Gorinov, D, Hall, J, Ignatiev, N, Ivanov, M, Jessup, K. L, Khatuntsev, I, Korablev, O, Kremic, T, Limaye, S, Lomakin, I, Martynov, A, Ocampo, A, Vaisberg, O, Voron, V, and Vorontsov, V

Subjects
Lunar And Planetary Science And Exploration
Abstract

Venus and Earth were formed approximately the same distance from the Sun, and have almost the same masses and volumes: they should be the most similar pair of planets in the Solar System. A vital, outstanding question is how and when these planets diverged in their atmospheric evolutions. Significantly, recent investigations present evidence for microbial life in Venus' cloud deck. Venus presents us with fundamental questions about the origin and evolution of planetary bodies and life in our Solar System.Venera-D (D stands for the Russian word for "long-lived:" dolgozhivushaya) is a potential mission that would combine simultaneous observations of Venus' atmosphere, plasma environment, and surface to try to answer these essential questions.

Published
2018

14. NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance

Author

Vandaele, A. C., Lopez-Moreno, J.-J., Patel, M. R., Bellucci, G., Daerden, F., Ristic, B., Robert, S., Thomas, I. R., Wilquet, V., Allen, M., Alonso-Rodrigo, G., Altieri, F., Aoki, S., Bolsée, D., Clancy, T., Cloutis, E., Depiesse, C., Drummond, R., Fedorova, A., Formisano, V., Funke, B., González-Galindo, F., Geminale, A., Gérard, J.-C., Giuranna, M., Hetey, L., Ignatiev, N., Kaminski, J., Karatekin, O., Kasaba, Y., Leese, M., Lefèvre, F., Lewis, S. R., López-Puertas, M., López-Valverde, M., Mahieux, A., Mason, J., McConnell, J., Mumma, M., Neary, L., Neefs, E., Renotte, E., Rodriguez-Gomez, J., Sindoni, G., Smith, M., Stiepen, A., Trokhimovsky, A., Vander Auwera, J., Villanueva, G., Viscardy, S., Whiteway, J., Willame, Y., Wolff, M., and the NOMAD Team

Published
2018
Full Text
View/download PDF

16. Martian Atmospheric Spectral End‐Members Retrieval From ExoMars Thermal Infrared (TIRVIM) Data

Author

Alemanno, G., D’Amore, M., Maturilli, A., Helbert, J., Arnold, G., Korablev, O., Ignatiev, N., Grigoriev, A., Shakun, A., Trokhimovskiy, A., 1 Institute for Planetary Research German Aerospace Center DLR Berlin Germany, 3 Space Research Institute (IKI) Moscow Russia, and 4 Australian National University Canberra ACT Australia

Subjects
Geophysics, ddc:523, Space and Planetary Science, Geochemistry and Petrology, TIRVIM data, Earth and Planetary Sciences (miscellaneous), Martian atmosphere
Abstract

Key knowledge about planetary composition can be recovered from the study of thermal infrared spectral range datasets. This range has a huge diagnostic potential because it contains diagnostic absorptions from a planetary surface and atmosphere. The main goal of this study is to process and interpret the dataset from the Thermal Infrared channel (TIRVIM) which is part of the Atmospheric Chemistry Suite of the ExoMars2016 Trace Gas Orbiter mission to find and characterize dust and water ice clouds in the atmosphere. The method employed here is based on the application of principal component analysis and target transformation techniques to extract the independent variable components present in the analyzed dataset. Spectral shapes of both atmospheric dust and water ice aerosols have been recovered from the analysis of TIRVIM data. The comparison between our results with those previously obtained on Thermal Emission Spectrometer (TES) data and with previous analysis on TIRVIM data, validates the methodology here applied, showing that it allows to correctly recover the atmospheric spectral endmembers present in the TIRVIM data. Moreover, comparison with atmospheric retrievals on PFS, TES and IRIS data, allowed us to assess the temporal stability and homogeneity of dust and water ice components in the Martian atmosphere over a time period of almost 50 years., Plain Language Summary: The analysis of thermal infrared datasets from planetary bodies is of key importance for the understanding of a planet's climate evolution and history: it contains valuable information about composition, temperature and state of the atmosphere. Moreover, surface properties and the surface‐atmosphere interaction can be studied. Here we investigated new thermal infrared data from the Thermal Infrared channel instrument of the ExoMars Trace Gas Orbiter with the main goal of carefully identifying Martian atmospheric dust and water ice clouds components. A methodology based on principal component and target transformation factor analysis techniques has been applied. Based on our results, this methodology can correctly recover both atmospheric dust and water ice aerosols spectral shapes and their abundances in the Martian atmosphere., Key Points: First successful application of principal components and target transformation techniques to high‐resolution Thermal Infrared channel (TIRVIM) data. Spectral shapes of both atmospheric dust and water ice clouds are recognized and recovered. TIRVIM data are successfully modeled through a linear combination of the recovered water ice and dust end‐members., Roscosmos and ESA, https://doi.org/10.5281/zenodo.7032738

Published
2022

19. Status report of the Venera-D Joint Science Definition Team

Author

Vorontsov, V, Vaisberg, O, Teselkin, S, Ocampo, A, Martynov, A, Lomakin, I, Limaye, S, Kremic, T, Korablev, O, Khatuntsev, I, Lea Jessup, K, Ivanov, M, Ignatiev, N, Hall, J, Gorinov, D, Gerasimov, M, Eismont, N, Economou, T, Burdanov, A, Zasova, L, and Senske, D

Abstract

UNKNOWN

Published
2017

20. Status report of the Venera-D Joint Science Definition Team

Author

Senske, D, Zasova, L, Burdanov, A, Economou, T, Eismont, N, Gerasimov, M, Gorinov, D, Hall, J, Ignatiev, N, Ivanov, M, Lea Jessup, K, Khatuntsev, I, Korablev, O, Kremic, T, Limaye, S, Lomakin, I, Martynov, A, Ocampo, A, Teselkin, S, Vaisberg, O, and Vorontsov, V

Published
2017

22. Martian Atmospheric Thermal Structure and Dust Distribution During the MY 34 Global Dust Storm From ACS TIRVIM Nadir Observations

Author

Vlasov, P., primary, Ignatiev, N., additional, Guerlet, S., additional, Grassi, D., additional, Korablev, O., additional, Grigoriev, А., additional, Shakun, A., additional, Patsaev, D., additional, Maslov, I., additional, Zasova, L., additional, Luginin, M., additional, Trokhimovskiy, A., additional, Millour, E., additional, Forget, F., additional, Haus, R., additional, Arnold, G., additional, and Montmessin, F., additional

Published
2022
Full Text
View/download PDF

23. The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter

Author

Korablev, O., Montmessin, F., Trokhimovskiy, A., Fedorova, A. A., Shakun, A. V., Grigoriev, A. V., Moshkin, B. E., Ignatiev, N. I., Forget, F., Lefèvre, F., Anufreychik, K., Dzuban, I., Ivanov, Y. S., Kalinnikov, Y. K., Kozlova, T. O., Kungurov, A., Makarov, V., Martynovich, F., Maslov, I., Merzlyakov, D., Moiseev, P. P., Nikolskiy, Y., Patrakeev, A., Patsaev, D., Santos-Skripko, A., Sazonov, O., Semena, N., Semenov, A., Shashkin, V., Sidorov, A., Stepanov, A. V., Stupin, I., Timonin, D., Titov, A. Y., Viktorov, A., Zharkov, A., Altieri, F., Arnold, G., Belyaev, D. A., Bertaux, J. L., Betsis, D. S., Duxbury, N., Encrenaz, T., Fouchet, T., Gérard, J.-C., Grassi, D., Guerlet, S., Hartogh, P., Kasaba, Y., Khatuntsev, I., Krasnopolsky, V. A., Kuzmin, R. O., Lellouch, E., Lopez-Valverde, M. A., Luginin, M., Määttänen, A., Marcq, E., Martin Torres, J., Medvedev, A. S., Millour, E., Olsen, K. S., Patel, M. R., Quantin-Nataf, C., Rodin, A. V., Shematovich, V. I., Thomas, I., Thomas, N., Vazquez, L., Vincendon, M., Wilquet, V., Wilson, C. F., Zasova, L. V., Zelenyi, L. M., and Zorzano, M. P.

Published
2017
Full Text
View/download PDF

26. O2 (а1Δg) Airglow at 1.27 μM and upper Mesosphere Dynamics on the Night Side of Venus.

Author

Shakun, A. V., Zasova, L. V., Gorinov, D. A., Khatuntsev, I. V., Ignatiev, N. I., Patsaeva, M. V., and Turin, A. V.

Subjects
MESOSPHERE, AIRGLOW, VENUSIAN atmosphere, VENUS (Planet), ATMOSPHERIC boundary layer
Abstract

This research studies the O2 (a1Δg) nightglow distribution in 1.27 μm to understand the dynamics of the atmosphere of Venus. Several factors were considered in the retrieval process, such as thermal emission of the lower atmosphere, reflection by the clouds. Results show deviation from SS-AS circulation mode: the area where horizontal flows from the dayside converge and where oxygen recombines and emits shifts from the midnight to 22–23 hours local time. This shift is caused by solar-induced thermal tide on Venus nightside. Some conclusions about the upper mesosphere dynamics are also presented. [ABSTRACT FROM AUTHOR]

Published
2023
Full Text
View/download PDF

27. Thermal Structure and Aerosols in Mars’ Atmosphere From TIRVIM/ACS Onboard the ExoMars Trace Gas Orbiter: Validation of the Retrieval Algorithm

Author

Guerlet, S., primary, Ignatiev, N., additional, Forget, F., additional, Fouchet, T., additional, Vlasov, P., additional, Bergeron, G., additional, Young, R. M. B., additional, Millour, E., additional, Fan, S., additional, Tran, H., additional, Shakun, A., additional, Grigoriev, A., additional, Trokhimovskiy, A., additional, Montmessin, F., additional, and Korablev, O., additional

Published
2022
Full Text
View/download PDF

32. AOST: Fourier spectrometer for studying mars and phobos

Author

Korablev, O. I., Grigor’ev, A. V., Moshkin, B. E., Zasova, L. V., Montmessin, F., Gvozdev, A. B., Shashkin, V. N., Patsaev, D. V., Makarov, V. S., Maksimenko, S. V., Ignatiev, N. I., Fedorova, A. A., Arnold, G., Shakun, A. V., Terentiev, A. I., Zharkov, A. V., Mayorov, B. S., Nikol’sky, Yu. V., Khatuntsev, I. V., Bellucci, G., Giuranna, M., Kuz’min, R. O., and Rodin, A. V.

Published
2012
Full Text
View/download PDF

33. New in the physics of planetary atmosphere

Author

Korablev, O. I., Zasova, L. V., Fedorova, A. A., Rodin, A. V., Ignatiev, N. I., Breus, T. K., Izakov, M. N., Maiorov, B. S., Krivolutsky, A. A., Petrova, E. V., Ivanov, A. Yu., and Trokhimovskii, A. Yu.

Published
2009
Full Text
View/download PDF

35. South-polar features on Venus similar to those near the north pole

Author

Piccioni, G., Drossart, P., Sanchez-Lavega, A., Hueso, R., Taylor, F. W., Wilson, C. F., Grassi, D., Zasova, L., Moriconi, M., Adriani, A., Lebonnois, S., Coradini, A., Bézard, B., Angrilli, F., Arnold, G., Baines, K. H., Bellucci, G., Benkhoff, J., Bibring, J. P., Blanco, A., Blecka, M. I., Carlson, R. W., Di Lellis, A., Encrenaz, T., Erard, S., Fonti, S., Formisano, V., Fouchet, T., Garcia, R., Haus, R., Helbert, J., Ignatiev, N. I., Irwin, P. G. J., Langevin, Y., Lopez-Valverde, M. A., Luz, D., Marinangeli, L., Orofino, V., Rodin, A. V., Roos-Serote, M. C., Saggin, B., Stam, D. M., Titov, D., Visconti, G., and Zambelli, M.

Published
2007
Full Text
View/download PDF

36. A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express

Author

Drossart, P., Piccioni, G., Gérard, J. C., Lopez-Valverde, M. A., Sanchez-Lavega, A., Zasova, L., Hueso, R., Taylor, F. W., Bézard, B., Adriani, A., Angrilli, F., Arnold, G., Baines, K. H., Bellucci, G., Benkhoff, J., Bibring, J. P., Blanco, A., Blecka, M. I., Carlson, R. W., Coradini, A., Di Lellis, A., Encrenaz, T., Erard, S., Fonti, S., Formisano, V., Fouchet, T., Garcia, R., Haus, R., Helbert, J., Ignatiev, N. I., Irwin, P., Langevin, Y., Lebonnois, S., Luz, D., Marinangeli, L., Orofino, V., Rodin, A. V., Roos-Serote, M. C., Saggin, B., Stam, D. M., Titov, D., Visconti, G., Zambelli, M., and Tsang, C.

Published
2007
Full Text
View/download PDF

37. First results of investigating the space environment onboard the Universitetskii-Tatyana satellite

Author

Sadovnichy, V. A., Panasyuk, M. I., Bobrovnikov, S. Yu., Vedenkin, N. N., Vlasova, N. A., Garipov, G. K., Grigorian, O. R., Ivanova, T. A., Kalegaev, V. V., Klimov, P. A., Kovtyukh, A. S., Krasotkin, S. A., Kuznetsov, N. V., Kuznetsov, S. N., Muravyeva, E. A., Myagkova, I. N., Pavlov, N. N., Nymmik, R. A., Petrov, V. L., Podzolko, M. V., Radchenko, V. V., Reisman, S. Ya., Rubinshtein, I. A., Riazantseva, M. O., Sigaeva, E. A., Sosnovets, E. N., Starostin, L. I., Sukhanov, A. V., Tulupov, V. I., Khrenov, B. A., Shakhparonov, V. M., Sheveleva, V. N., Shirokov, A. V., Yashin, I. V., Markelov, V. V., Ivanov, N. N., Blinov, V. N., Sedykh, O. Yu., Pinigin, V. P., Papkov, A. P., Levin, E. S., Samkov, V. M., Ignatiev, N. N., and Yamnikov, V. S.

Published
2007
Full Text
View/download PDF

39. 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

Author

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., and Ekonomov, A. P.

Published
2006
Full Text
View/download PDF

41. Venus Monitoring Camera for Venus Express

Author

Markiewicz, W.J., Titov, D.V., Ignatiev, N., Keller, H.U., Crisp, D., Limaye, S.S., Jaumann, R., Moissl, R., Thomas, N., Esposito, L., Watanabe, S., Fiethe, B., Behnke, T., Szemerey, I., Michalik, H., Perplies, H., Wedemeier, M., Sebastian, I., Boogaerts, W., Hviid, S.F., Dierker, C., Osterloh, B., Böker, W., Koch, M., Michaelis, H., Belyaev, D., Dannenberg, A., Tschimmel, M., Russo, P., Roatsch, T., and Matz, K.D.

Published
2007
Full Text
View/download PDF

44. Phyllosilicates on Mars and implications for early martian climate

Author

Poulet, F., Bibring, J.-P., Mustard, J. F., Gendrin, A., Mangold, N., Langevin, Y., Arvidson, R. E., Gondet, B., Gomez, C., Berthe, M., Erard, S., Forni, O., Manaud, N., Poulleau, G., Soufflot, A., Combes, M., Drossart, P., Encrenaz, T., Fouchet, T., Melchiorri, R., Bellucci, G., Altieri, F., Formisano, V., Fonti, S., Capaccioni, F., Cerroni, P., Coradini, A., Korablev, O., Kottsov, V., Ignatiev, N., Titov, D., Zasova, L., Pinet, P., Schmitt, B., Sotin, C., Hauber, E., Hoffmann, H., Jaumann, R., Keller, U., Arvidson, R., Mustard, J., and Forget, F.

Abstract

Author(s): F. Poulet (corresponding author) [1]; J.-P. Bibring [1]; J. F. Mustard [2]; A. Gendrin [2]; N. Mangold [3]; Y. Langevin [1]; R. E. Arvidson [4]; B. Gondet [1]; C. [...]

Published
2005
Full Text
View/download PDF

45. The planetary fourier spectrometer (PFS) onboard the European Venus Express mission

Author

Formisano, V., Angrilli, F., Arnold, G., Atreya, S., Baines, K.H., Bellucci, G., Bezard, B., Billebaud, F., Biondi, D., Blecka, M.I., Colangeli, L., Comolli, L., Crisp, D., D’Amore, M., Encrenaz, T., Ekonomov, A., Esposito, F., Fiorenza, C., Fonti, S., Giuranna, M., Grassi, D., Grieger, B., Grigoriev, A., Helbert, J., Hirsch, H., Ignatiev, N., Jurewicz, A., Khatuntsev, I., Lebonnois, S., Lellouch, E., Mattana, A., Maturilli, A., Mencarelli, E., Michalska, M., Lopez Moreno, J., Moshkin, B., Nespoli, F., Nikolsky, Yu., Nuccilli, F., Orleanski, P., Palomba, E., Piccioni, G., Rataj, M., Rinaldi, G., Rossi, M., Saggin, B., Stam, D., Titov, D., Visconti, G., and Zasova, L.

Published
2006
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results