Changes in meteorological parameters during the total solar eclipse of 2 July 2019 in La Serena, Chile

被引:2
|
作者
Lazzus, Juan A. [1 ,2 ]
Vega-Jorquera, Pedro [1 ]
Pacheco, Rene [1 ]
Tamblay, Luis [1 ]
Martinez-Ledesma, Miguel [3 ,4 ]
Ovalle, Elias M. [4 ,5 ]
Carrasco, Enrique [4 ,6 ]
Bravo, Manuel [4 ,6 ]
Villalobos, Carlos U. [4 ,6 ]
Salfate, Ignacio [1 ]
Palma-Chilla, Luis [1 ]
Foppiano, Alberto J. [5 ]
机构
[1] Univ La Serena, Dept Fis, Casilla 554, La Serena, Chile
[2] Univ La Serena, Inst Invest Multidisciplinario Ciencias & Tecnol, La Serena, Chile
[3] Univ Concepcion, Dept Astron, CePIA, Concepcion, Chile
[4] Ctr Interuniv Fis Alta Atmosfera, CInFAA, Concepcion, Chile
[5] Univ Concepcion, Dept Geofis, Concepcion, Chile
[6] Univ Adventista Chile, Ctr Instrumentac Cient, Chillan, Chile
关键词
Total solar eclipse; Surface solar radiation; Solar-terrestrial interaction; Micrometeorology; Energy balance; 11; AUGUST; 1999; SURFACE-ENERGY FLUXES; MARCH; 2006; OZONE CONCENTRATION; AIR-TEMPERATURE; WIND-SPEED; NY-ALESUND; IMPACTS; IRRADIANCE; EVOLUTION;
D O I
10.4401/ag-8623
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The first report on the changes in meteorological parameters during the total solar eclipse of July 2, 2019, in La Serena (Chile), is presented. The event could be observed from morning time on the east of New Zealand, in the South Pacific Ocean, to sunset time in Chile. Several meteorological properties such as global radiation Rg, net radiation Rn, reflected radiation Rr (in Wm-2/min), air temperature (TA in degrees C), relative humidity (RH in %), wind speed amplitude (WS in ms-1), and wind speed direction (WD in degrees), were recorded with La Serena weather station SER (29.827 degrees S, 71.261 degrees W, 28 masl) at 1-minute time resolution. Importantly, SER was located at 40 km from the axis of the umbra that covered 201 km of width, where it reached 100% darkness at a magnitude of 1.009 during a clear-sky day. Under these auspicious conditions, we observed a rate of changes in the drop of the radiation components of 3.1, 2.4, and 0.5 (Wm-2/min) for Rg, Rn, and Rr, respectively, with a 100% reduction in the components of surface solar radiation (0 Wm-2) during totality. In addition, all components showed a-34% energy loss during the eclipse in comparison with the day before the event. Also, the rate of changes of -3.3 degrees C in TA, +11% in RH, -1.11 ms-1 in WS, and 180 degrees to 340 degrees for WD in total synchrony with the passing of the moon in front of the sun, reaching respective peaks at-5 min lag with respect to totality. Thus, our results show a progressive change in all meteorological parameters in total synchrony with the eclipse's phases caused by the passing of the moon in front of the sun.
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页数:17
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