학술논문
Dataset of night-time emissions of the Earth in the near UV range (290-430 nm), with 6.3 km resolution in the latitude range -51.6
Document Type
article
Author
L. Marcelli; K. Bolmgren; D. Barghini; M. Battisti; C. Blaksley; S. Blin; A. Belov; M. Bertaina; M. Bianciotto; F. Bisconti; G. Cambiè; F. Capel; M. Casolino; I. Churilo; M. Crisconio; C. De La Taille; T. Ebisuzaki; J. Eser; F. Fenu; M.A. Franceschi; C. Fuglesang; A. Golzio; P. Gorodetzky; H. Kasuga; F. Kajino; P. Klimov; V. Kuznetsov; M. Manfrin; G. Mascetti; W. Marszal; H. Miyamoto; A. Murashov; T. Napolitano; H. Ohmori; A. Olinto; E. Parizot; P. Picozza; L.W. Piotrowski; Z. Plebaniak; G. Prevot; E. Reali; G. Romoli; M. Ricci; N. Sakaki; K. Shinozaki; J. Szabelski; Y. Takizawa; V. Vagelli; G. Valentini; M. Vrabel; L. Wiencke
Source
Data in Brief, Vol 48, Iss , Pp 109105- (2023)
Subject
Language
English
ISSN
2352-3409
Abstract
The data presented in this article are related to the research paper entitled “Observation of night-time emissions of the Earth in the near UV range from the International Space Station with the Mini-EUSO detector” (Remote Sensing of Environment, Volume 284, January 2023, 113336, https://doi.org/10.1016/j.rse.2022.113336).The data have been acquired with the Mini-EUSO detector, an UV telescope operating in the range 290-430 nm and located inside the International Space Station. The detector was launched in August 2019, and it has started operations from the nadir-facing UV-transparent window in the Russian Zvezda module in October 2019. The data presented here refer to 32 sessions acquired between 2019-11-19 and 2021-05-06. The instrument consists of a Fresnel-lens optical system and a focal surface composed of 36 multi-anode photomultiplier tubes, each with 64 channels, for a total of 2304 channels with single photon counting sensitivity. The telescope, with a square field-of-view of 44°, has a spatial resolution on the Earth surface of 6.3 km and saves triggered transient phenomena with a temporal resolution of 2.5 µs and 320 µs. The telescope also operates in continuous acquisition at a 40.96 ms scale.In this article, large-area night-time UV maps obtained processing the 40.96 ms data, taking averages over regions of some specific geographical areas (e.g., Europe, North America) and over the entire globe, are presented. Data are binned into 0.1° × 0.1° or 0.05° × 0.05° cells (depending on the scale of the map) over the Earth's surface. Raw data are made available in the form of tables (latitude, longitude, counts) and .kmz files (containing the .png images). These are – to the best of our knowledge – the highest sensitivity data in this wavelength range and can be of use to various disciplines.