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.
引用
收藏
页数:17
相关论文
共 50 条
  • [31] Interpretation of the tidal residuals during the 11 July 1991 total solar eclipse
    Ducarme, B
    Sun, HP
    d'Oreye, N
    Van Ruymbeke, M
    Jara, JM
    JOURNAL OF GEODESY, 1999, 73 (02) : 53 - 57
  • [32] Interpretation of the tidal residuals during the 11 July 1991 total solar eclipse
    B. Ducarme
    H.-P. Sun
    N. d'Oreye
    M. Van Ruymbeke
    J. Mena Jara
    Journal of Geodesy, 1999, 73 : 53 - 57
  • [33] OPTICAL POLARIZATION OBSERVATIONS OF THE SOLAR CORONA DURING THE TOTAL SOLAR ECLIPSE OF 1991 JULY 11
    TANABE, T
    TSUMURAYA, F
    BABA, N
    ALVAREZ, M
    NOGUCHI, M
    ISOBE, S
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1992, 44 (05) : L221 - L226
  • [34] INFRARED RADIOMETRIC OBSERVATIONS OF SOLAR CORONA DURING TOTAL SOLAR ECLIPSE OF 20 JULY 1963
    TAYLOR, JH
    MACQUEEN, RM
    APPLIED OPTICS, 1964, 3 (12): : 1365 - &
  • [35] CHANGES IN THE CONCENTRATION OF MESOSPHERIC OZONE DURING THE TOTAL SOLAR ECLIPSE
    AGASHE, VV
    RATHI, SM
    PLANETARY AND SPACE SCIENCE, 1982, 30 (05) : 507 - 513
  • [36] Visible Emission Line Spectroscopy of the Solar Corona During the 2019 Total Solar Eclipse
    Gabriel D. Muro
    Matt Gunn
    Stephen Fearn
    Tomos Fearn
    Huw Morgan
    Solar Physics, 2023, 298
  • [37] Visible Emission Line Spectroscopy of the Solar Corona During the 2019 Total Solar Eclipse
    Muro, Gabriel D.
    Gunn, Matt
    Fearn, Stephen
    Fearn, Tomos
    Morgan, Huw
    SOLAR PHYSICS, 2023, 298 (06)
  • [38] AIR-TEMPERATURE AND WIND CHANGES IN COSTA-RICA DURING THE TOTAL SOLAR ECLIPSE OF JULY 11, 1991
    FERNANDEZ, W
    CASTRO, V
    HIDALGO, H
    EARTH MOON AND PLANETS, 1993, 63 (02): : 133 - 147
  • [39] Spectroscopic Observation of Oscillations in the Corona During the Total Solar Eclipse of 22 July 2009
    Jagdev Singh
    S. S. Hasan
    G. R. Gupta
    K. Nagaraju
    D. Banerjee
    Solar Physics, 2011, 270
  • [40] Spectroscopic Observation of Oscillations in the Corona During the Total Solar Eclipse of 22 July 2009
    Singh, Jagdev
    Hasan, S. S.
    Gupta, G. R.
    Nagaraju, K.
    Banerjee, D.
    SOLAR PHYSICS, 2011, 270 (01) : 213 - 233