Bharat mein teen laghu akshaansh kendron ke oopar ozone ke oordhvaadhar vitaran kee ozone sonde aankadon ke dvaara pradarshit pravrtti
DOI:
https://doi.org/10.54302/mausam.v67i2.1354Keywords:
Vertical distribution, Solar activity, Ultraviolet radiation, AtmosphereAbstract
This study examines the trends in the vertical distribution of ozone over three low latitude stations in India. The stations are Delhi (28° N, 77° E), Pune (18° N, 74° E) and Thiruvananthapuram (8° N, 76° E) lying in the almost same longitude belt (74-77°) but separated by10o latitude. The balloon ozonesonde data of 45 years (1969 – 2012) have been analyzed. It has been found that ozone trends at different altitudes are different for three stations. The peak value and the altitude of peak value vary from year to year. This is due to solar UV-B variation.
Downloads
Published
How to Cite
Issue
Section
License
Copyright (c) 2021 MAUSAM
This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
All articles published by MAUSAM are licensed under the Creative Commons Attribution 4.0 International License. This permits anyone.
Anyone is free:
- To Share - to copy, distribute and transmit the work
- To Remix - to adapt the work.
Under the following conditions:
- Share - copy and redistribute the material in any medium or format
- Adapt - remix, transform, and build upon the material for any purpose, even
commercially.
