atmospheric effects in the electromagnetic component of the secondary cosmic rays in the pierre...
TRANSCRIPT
Atmospheric Effects in the Electromagnetic Component of
the Secondary Cosmic Rays in the Pierre Auger Observatory
J. Alvarez-Castillo1 and J. F. Valdés-Galicia1, for the Pierre Auger Collaboration2
IS@O, April 2011
1 Space Sciences, Geophysical Institute, UNAM, Mexico City, Mexico.
2 Pierre Auger Observatory, Malargüe, Mendoza, Argentina.
History
Alexeenko et al. 1985, 2002
1985:−1% hard + 2% soft
2002: Different effects for hard and soft components.
Muraki et al., 2004The increase of the counting rate was only about 1%.
Aglietta et al., 1999Increase of 5% of the counting rate.
González & Valdés-Galicia, 2006Alvarez-Castillo & Valdés-Galicia, 2010Variations of ±0.5-1% of the counting rates on average for hard and soft components.
Alvarez-Castillo & Valdés-Galicia, this work
The increase of the counting rate was only about 1%.
The Pierre Auger Observatory
The Pierre Auger Observatory is located in the Southern Hemisphere, in the area of Malargüe city, Mendoza Province, Argentina.
The Auger Observatory consists of an array of 1,600 water Cherenkov detectors, on a 1.5 km in an hexagonal grid covering 3,000 km2. The surface detector network is complemented by fluorescence detectors and weather stations.
EF during Thunderstorms(TS) >1,000 V/m, EF in Quiet Days (QD) < 200 V/m.
Fluctuations are different: In QD the most important variation is the diurnal variation. In TS both disturbances are coupled.
Red= Electric Field (EF); Blue= CR (Cosmic Rays)
Thunderstorm
Quiet Day
Data Selection
1. CR close to the solar minimum (2007/11/27-2010/01/22).
2. Data with large variations in the geomagnetic field (kp > 20) and Forbush decreases were discarded.
3. Correction for pressure was made, other effects were not considered, as they are of minor importance.
4. TS were defined as measurements of |EF| > 800 V/m.
5. QD were selected considering measurements of |EF| < 200 V/m.
6. WD are considered with measurements of 200 < |EF| < 800 V/m.
7. Other atmospheric variables were considered (temperature, pressure and humidity).
8. Data resolution for this study is five minutes.
Methodology
All data during electric storms, quiet and windy days were filtered, removing the lowest frequencies.
An analysis of frequency-time (wavelet) was performed to the data, obtaining the periodicities of these.
Signals were compared in time and frequency.
One second SD scaler data were processed to eliminate anomalies due to jumps in the PMT baselines(Not considered in this presentation).
Filtered CR data (five minute resolution)
The Filtering of the CR data during a day with a thunderstorm (2007/12/25), is shown in the bottom panel, the two sigma level is exceeded from 13:45 to 19:10 UTC, when a TS occurred.
Trend
Original data
Filtered
2 σInterval of the effects of the Thunderstorm
Wavelet Spectrum
Note:
-Red noise is calculated dynamically considering each time series.
-Sigma normalization data.
Interval of the TS effects on the EM component
Time serie of normalized data
Spectrogram
highest power
lowest power
red noise
Wavelet analysis during thunderstorms (five minute resolution 25/12/2007)
Peaks in the Spectrum are at 5 hr, 2 hr and also around 30 min. Beyond 15 min. the signal is confused with the red noise level.
EF spectrum shows two peaks: one with a maximum around 30-45 min., another around 6 hours, below the red noise.
FLUCTUATIONS ARE MUCH STRONGER DURING TS
Temperature Humidity Pressure
Electric Field Cosmic Rays Wind Speed
Wavelet analysis in quiet days(five minute resolution 20/03/2008)
Two peaks are present: around 30 min and one hour. Other two peaks are close to the red noise level: 3.15 hours and 6 hours.
Periodicities in EF are: one around 20 minutes, another from 4 to 6 hours (maximum at 5 hours), and a small peak close to 3 hours.
FLUCTUATIONS ARE SPARSE,
HF IS UNCORRELATED
Temperature Humidity Pressure
Electric Field Cosmic Rays Wind Speed
Filtered data (2007/12/08)
Cosmic Rays
Electric Field
Wind Speed
Temperature
Relative Humidity
Pressure
Temperature Humidity Pressure
Electric Field Cosmic Rays Wind Speed
CR and EF summary
CR (hours) EF (hours)
< 0.5 < 0.5
0.5, 1 0.5-1
2 (not always), ~5 2 (not always), ~5
Quiet days:
HF VARIATIONS ARE UNCORRELATED.
Periodicities present:
Thunderstorms days:
WE SEE HARMONIC VARIATIONS
IN CR AND EF (TUNED)
Periodicities present:
CR (hours) EF (hours)
< 0.5 < 0.5
0.5, 1 0.5-1
2 (not always), ~4-5 2 (not always), ~4-5
We worked with 12 TS and 21 QD
Possible explanations for periodicities
The periodicities of 30min, in CR and EF could be related to electric field transitions, known to exist higher in the atmosphere (Israel, 1971)
The periodicities of half hour and less in EF and CR, with some intermittency, may be connected with microburst wind, that potentially carries large amounts of dust, whose composition in Malargüe is mostly iron (FIP 8 eV), that could be electrically charged (Rasmussen et al., 2009).
The 2 hour periodicity in CR and EF could be related to light and gentle wind, carrying charged particles and ions (Reiter, 1992). The CR variation of around 6 hours is due to the fourth harmonic diurnal variation of the EF.(Bhartendu, 1972).
Other low frequency variations in CR during TS may be due to rain. Rain droplets carry unstable particles that decay and contribute to changes in the flow of the CR; for this reason these variations are not present in the EF [Aglietta et al., 1999; Vernetto , 2001; Alexeenko et al., 2007].
The main contributions of this work are:
1. During thunderstorms electric field and cosmic rays variations are coupled.
2. The variations in the electric field are composed of two frequencies: a high frequency of a few minutes and a low frequency of a few hours.
The high frequency is intermittent and is due to the existence of high intensity EF (higher than ±4,000 V/m) during thunderstorms.
The low frequency may be connected to the wind flow that carries particles and ions that build the EF, it is present in QD. The atmospheric electric field is, to a significant extent, due to charged particles and ions in the air, that generally tend to have a net positive charge (Reiter, 1992).
3. The intermittent EF and CR fluctuations that are coincident may be connected with microburst wind, that potentially carries large amounts of dust and ions. (Rasmussen et al., 2009)
SUMMARY
Acknowledgments
The successful installation and commissioning of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe.
M. in P. Hernán Asorey and Dr. Xavier Bertou for technical support in the Auger observatory data in the Centro Atómico Bariloche (San Carlos de Bariloche, Río Negro, Argentina).
CONACYT (Consejo Nacional de Ciencia y Tecnología) for the scholarship awarded me for the completion of doctoral.
We are very grateful to the following agencies and organizations for financial support in the Pierre Auger Observatory:
Thank you very much for your kind attention!
Tank selection for one second data resolution
Wavelet analysis during thunderstorm(one second resolution)
SCR Global spectrum at high frequencies
Periodicities of 0-90 seconds
Periodicities of 0-20 seconds
Periodicities summary (secs)
Tank Below red noise level Close to red noise level Above red noise level
323 12, 20 3.5, 7.6 40
373 2.5, 7.5, 16, 24, 40 5
472 3.5, 30 8
479 2.5, 5, 10, 14 22, 48
577 2.5, 30, 64 6 12
701 3, 16, 26, 40 12
875 3.5, 6, 28 12 50
901 6, 10-14, 24, 50 3.5
974 2.8, 4, 12, 25, 50 7
1034 2.5-3.5, 4, 8-12, 19, 32
1053 2.5, 5, 6.5 16 32
1101 3.8, 7, 14, 19, 30
1198 3.8, 6, 12, 25 38
1365 3, 5, 12-14, 24-28, 32-44, 58-64 16
1605 2.5-4, 8, 13, 16, 28, 58
Electric field spectrum
The periodicities ranging from 4 to 64 seconds!!
Preliminary Results(one second resolution)
Temporal resolution data of a second are useful to see the effects of lightning on the electromagnetic component of cosmic rays.
Very large increases covering a range from 5-25 standard deviations, depending of the intensity of the discharge.
Much of the variation present in cosmic rays are caused by an electric effect, which can be: redistributions of charges, electric shock or resonant effects, in the range of 4-64 seconds.
Periodicities<4 sec in SCR, are possibly due to the Runaway Breakdown Process. The presence of a strong electric field in a thundercloud causes the acceleration of energetic electrons, which through collisions generate more fast electrons, which in turn will be also accelerated, causing a cascading effect that leads to a large flow of electrons producing the electric discharge (Gurevich et al, 1999).
A partir de un campo eléctrico de alta tensión, nace la A partir de un campo eléctrico de alta tensión, nace la formación de la descargaformación de la descarga
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Departamento de Ciencias Espaciales
La constante de Ionizacion del aire
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Genera una concentración de cargas puntual, donde aparecen los trazadores
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y abren el camino ionizado de conexión, y la descarga eléctrica aparece
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El aire queda saturado eléctricamente
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Departamento de Ciencias Espaciales
Y el proceso se puede repetir mas rápidamente
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Departamento de Ciencias Espaciales
Teniendo varias descargas, lo cual esta en función de la carga de la nube
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Departamento de Ciencias Espaciales
Distribución Mundial de Descargas Eléctricas
Diariamente en el mundo se producen unas 44,000 tormentas y se generan mas de 8,000,000 de descargas
Departamento de Ciencias Espaciales
Curva de Carnegie según LIS
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Tank You very much !!!Tank You very much !!!