title: ÐÐ¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¾Ð±ÑÑÑÐ½ÐµÐ½Ð¸Ñ ÑÐµÐ·Ð¾Ð½Ð½ÑÑ Ð²Ð°ÑÐ¸Ð°ÑÐ¸Ð¹ ÐºÐ¸ÑÐ»Ð¾ÑÐ¾Ð´Ð° Ð² Ð°ÑÐ¼Ð¾ÑÑÐµÑÐµ ÐÐ°ÑÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Possible explanations for seasonal variations of oxygen in the Martian atmosphere
Creators: name: ÐÐµÑÐºÑÐ»Ð¾Ð²Ð°, ÐÐ»Ð¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: ÐÐ¸ÑÐ»Ð¾ÑÐ¾Ð´
ÐÑÐ¼Ð¾ÑÑÐµÑÐ° Ð¿Ð»Ð°Ð½ÐµÑ
Ð¡Ð¾Ð»Ð½ÐµÑÐ½Ð°Ñ ÑÐ°Ð´Ð¸Ð°ÑÐ¸Ñ
ÐÐ·Ð¾Ð½
ÐÐ°ÑÑ
ÐºÐ»Ð°ÑÑÐ°Ñ
ÑÐ¾ÑÐ¾Ñ Ð¸Ð¼Ð¸Ñ
ÑÐ¾ÑÐ¾Ð´Ð¸ÑÑÐ¾ÑÐ¸Ð°ÑÐ¸Ñ
Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ»ÐµÐ²Ð°Ñ Ð±ÑÑÑ
ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÐ¹ ÑÐ¸ÐºÐ»
Mars
clathrate
photochemistry
photodissociation
global dust storm
solar cycle

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿Ð¾Ð¸ÑÐºÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ° ÑÐµÐ·Ð¾Ð½Ð½ÑÑ Ð²Ð°ÑÐ¸Ð°ÑÐ¸Ð¹ ÐºÐ¸ÑÐ»Ð¾ÑÐ¾Ð´Ð° Ð² Ð°ÑÐ¼Ð¾ÑÑÐµÑÐµ ÐÐ°ÑÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð±ÑÐ»Ð¸ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ° Ð²Ð°ÑÐ¸Ð°ÑÐ¸Ð¹ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ»Ð°ÑÑÐ°ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ Ð¡Ð2+Ð3+Ð2 Ð¼Ð°ÑÑÐ¸Ð°Ð½ÑÐºÐ¾Ð¹ Ð·Ð¸Ð¼Ð¾Ð¹ Ð² Ð¿Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ°Ð¿ÐºÐ°Ñ. Ð¢Ð°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð´Ð¸Ñ Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð¸Ðµ Ð¾Ð·Ð¾Ð½Ð°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð²Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ð¸ Ð²ÐµÑÐ½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¾ÑÐ¸Ð¸ÑÑÐµÑ Ð´Ð¾ ÐºÐ¸ÑÐ»Ð¾ÑÐ¾Ð´Ð°. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¾ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÐºÐ»Ð°ÑÑÐ°ÑÐ° Ð¸ ÐºÐ¾ÑÑÐµÐ»ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð²Ð»Ð¸ÑÑÑÐ¸Ñ Ð½Ð° ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ñ Ð¾Ð·Ð¾Ð½Ð°. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ, Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑÐ¸Ðµ, ÑÑÐ¾ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐ¹ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ ÑÐ²Ð»ÑÐµÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐ¼ Ð¾Ð±ÑÑÑÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð½ÑÑ Ð²Ð°ÑÐ¸Ð°ÑÐ¸Ð¹ ÐºÐ¸ÑÐ»Ð¾ÑÐ¾Ð´Ð° Ð² Ð°ÑÐ¼Ð¾ÑÑÐµÑÐµ ÐÐ°ÑÑÐ°. Ð Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ¼ ÑÑÐµÐ±ÑÐµÑÑÑ ÑÑÐµÑÐ¼ÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ ÑÑÐµÑÐ¾Ð¼ Ð¿ÐµÑÐµÐ½Ð¾ÑÐ°, ÑÑÐ¾ÐºÐ° Ð¸ Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð¸Ñ Ð¾Ð·Ð¾Ð½Ð° Ð² Ð¿Ð¾Ð»ÑÑÐ½ÑÑ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ñ Ð´Ð»Ñ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¾ÑÐ¸Ð¸.
description: The given work is devoted to the search for a possible source of seasonal variations of oxygen in the atmosphere of Mars, which were discovered experimentally. The formation of the clathrate compound CO2+O3+O2 in the Martian winter in the polar caps is considered as a possible source of variations. Thus, ozone accumulates, which subsequently dissociates to oxygen in the spring. The study was conducted based on a thermodynamic clathrate model and a correlation analysis of processes affecting ozone concentration. As a result, calculations were carried out showing that the proposed mechanism is a possible explanation for the detected oxygen variations in the Martian atmosphere. In the future, three-dimensional modeling is required, considering the transport, runoff, and accumulation of ozone in the polar regions to confirm the developed theory.