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Bibring J.-P., Langevin Y., Gendrin A., Gondet B., Poulet F., Berth M., Soufflot A., ErardS., FomiO., ArvidsonR., MangoldN., MustardJ., DrossartP., CombesM., EncrenazT., FouchetT., MerchiorriR., BelluciG., AltieriF., FormisanoV., Bonello G., Capaccioni F., Cerroni P., Coradini A., Fonti S., Kottsov V., Ignatiev N., MorozV., TitovD., ZasovaL., PinetP., DoutS., SchmittB., SotinC., HauberE., Hoffmann H., Jaumann R., Keller U., Duxbury T., Forget F. Mars Surface Diversity as Revealed by the Omega/Mars Express Observations //Sciences.


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V.125. P.212229. (43) Sagdeev R. Z., Avanesov G. A., Barinov I. V., Debabov A. I., Kvasikov V. A., Moroz V. I. Comet Halley: Nucleus And Jets (Results of The Vega Mission) // Advances in Space Research (includes Cospar Information Bulletin).

1985. V.5. N.12. P.95. (3) SagdeevR. Z., BlamontJ., GaleevA. A., MorozV. I., ShapiroV. D., ShevchenkoV. I., Szego K. Vega Spacecraft Encounters with Comet Halley // Nature. 1986.

V.321. P.259262. (25) SagdeevR. Z., ElyasbergP. E., MorozV. I. Is the Nucleus of Comet Halley a Low Density Body? //Nature. 1988. V.331. P.240. (22) Schafer K., Dubois R., Haus R., Dethloff K., Goering H., Oertel D., Becker-Ross H., StadthausW., SpankuchD., MorozV. I., ZasovaL. V., MatsygorinI. A. Infrared Fourier Spectrometer Experiment from Venera-15 // Advances in Space Research (includes Cospar Information Bulletin). 1990. V.10. N.5. P.57. (8) Seiff A., Schofield J. T., Kliore A., Taylor F. W., Limaye S. S., Revercomb H. E., Sromovsky L. A., Kerzhanovich V. V., Moroz V. I., Marov M. Ya. Models of the structure of the atmosphere of Venus from the surface to 100kilometers altitude //Advance in Space Research. 1985. V.5(11). P.358.

Snyder C. W., Moroz V. I. Spacecraft exploration of Mars // Mars / Eds. Kieffer H. H., Jakosky B. M., Snyder C. W., Matthews M. S. Tucson, London: The University of Arizona Press, 1992. P.71119.

Titov D. V., Baines K. H., Crisp D., Basilevsky A. T., Chassefiere E., Chin G., Esposito L. W., Lebreton J. P., Lellouch E., Moroz V. I., Nagy A. F., Owen T. C., OyamaK. I., RussellC. T., TaylorF. W., YoungR. E. Missions to Venus //European Space Agency (Special Publication): ESA SPProceedings of the 36th ESLAB Symposium; Earth-Like Planets and Moons / Eds. B. Foing, B. Battrick.

Noordwijk, 2002. P.1320. (4) TitovD. V., MorozV. I., GektinYu. M. Aerosol component of the Martian atmosphere and its variability from the results of infrared radiometry in the Termoscan/Phobos-2 experiment //Planetary and Space Science. June 1997.

V.45. Iss.6. P.637651. (9) Titov D. V., Moroz V. I., GrigorievA. V., RosenqvistJ., CombesM., BibringJ. P., Arnold G. Observations of water vapour anomaly above Tharsis volcanoes on Mars in the ISM (Phobos-2) experiment //Planetary and Space Science.

November 1994. V.42. Iss.11. P.10011010. (19) TitovD. V., RosenqvistJ., MorozV. I., GrigorievA. V., ArnoldG. Evidences of the Regolith-Atmosphere Water Exchange on Mars from the ISM (Phobos-2) Infrared Spectrometer Observations // Advances in Space Research (includes Cospar Information Bulletin). 1995. V.16. N.6. P.23. (14) UstinovE. A., MorozV. I. An Attempt to Improve the H2O Content in the Atmosphere of Venus from the Narrow Band Photometry Aboard the Venera9 and Venera10 Probes //Cosmic Research. 1978. .16. .127. (2) Venus /Eds. HuntenD. M., ColinL., DonahueT. M., MorozV. I. The University of Arizona Press, Tucson. 1983. 1143p.

Venus international reference atmosphere /Eds. KlioreA. J., MorozV. I., KeatingG. M. //Advances in Space Research (ASR). 1985. V.5. N.11. 305p.

VonZahn U., MorozV. I. Composition of the Venus atmosphere below 100km altitude //Venus International Reference Atmosphere /Ed. KlioreA. J., MorozV. I. KeatingG. M. Advance Space Research. 1985. V.5. P.173196.

Zasova L., Khatountsev I. V., Ignatiev N. I., Moroz V. I. Local Time Variations of the Middle Atmosphere of Venus: Solar-Related Structures //Advances in Space Research (includes Cospar Information Bulletin). 2002. V. 29. N. 2.

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Zasova L. V., Ignantiev N. I., Moroz V. I., Formisano V., Grassi D. Thermal Structure of the Martian Atmosphere Retrieved from the IR Spectrometry in the 15 m CO2 Band: Input to Mira // Advances in Space Research (includes Cospar Information Bulletin). 2005. V.35. N.1. .813. (5) ZasovaL. V., IgnatevN. I., MorozV. I., KhatuntsevI. V. Venera-15: Water Vapor at Altitudes of 5565km //Cosmic Research. 1999. V.37. N.1. P.2730. (1) Zasova L. V., Khatountsev I. V., Moroz V. I. Ignatiev N. I. Structure of the Venus Middle Atmosphere: Venera 15 IR Fourier Spectrometry Data Revisited //Advances in Space Research. 1999. V.23. N.9. P.15591568. (20) Zasova L. V., Krasnopolsky V. A., Moroz V. I. Vertical Distribution of SO2 in the Upper Cloud Layer of Venus and Origin of UV Absorption //Advances in Space Research (includes Cospar Information Bulletin). 1981. V.1. P.13. (2) Zasova L. V., Moroz V. I. Latitude Structure of Upper Clouds of Venus // Advances in Space Research (includes Cospar Information Bulletin). 1992.

V.12. N.9. P.7990.(6) ZasovaL. V., MorozV. I., EspositoL. W., NaC. Y. SO2 in the Middle Atmosphere of Venus: IR Measurements from Venera-15 and Comparison to UV Data //Icarus. 1993. V.105. P.92. (26) ZasovaL. V., MorozV. I., FormisanoV. etal. Infrared spectrometry of Venus: IR Fourier Spectrometer on Venera15 as a precursor of PFS for Venus Express //Advances in Space Research. 2004. V.34. P.16551667. (10) ZasovaL. V., MorozV. I., IgnatievN. I., GnedykhV. N., GrigorievA. V., MoshkinB. E., Nikolsky Yu. V., Patsaev D. V., Khatuntsev I. V., Ekonomov A. P., Formisano V., GrassiD., GiurannaM., BellucciG., AltieriF., MattanaA., MaturilliA., BibringJ.P., Blecka M., Ratai M. et al. 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 // Cosmic Research. 2006. V.44. N.4. .305316. (3) ZasovaL. V., MorozV. I., IgnatievN. I., KhatuntsevI. V., FormisanoV. Exploration of Venus with the Venera-15 IR Fourier Spectrometer and the Venus Express Planetary Fourier Spectrometer //Cosmic Research. 2006. V.44. N.4.

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