scholarly journals MoCRiS a low-cost stratospheric balloon platform to measure the particle flux of cosmic ray showers in the high atmosphere.

2021 ◽  
Author(s):  
Valerio Bocci ◽  
Antonino Brosio ◽  
Gabriele Galbato Muscio ◽  
Francesco Iacoangeli ◽  
Domenico Liguori ◽  
...  
2019 ◽  
Author(s):  
Erika Brattich ◽  
Encarnación Serrano Castillo ◽  
Fabrizio Giulietti ◽  
Jean-Baptiste Renard ◽  
Sachi N. Tripathi ◽  
...  

Abstract. This paper describes the aerosol measurements setup and results obtained during the BEXUS18 stratospheric balloon within the A5-Unibo (Advanced Atmospheric Aerosol Acquisition and Analysis) experiment performed on October 10th, 2014 in northern Sweden (Kiruna). The experimental setup was designed and developed by the University of Bologna with the aim of collecting and analyzing vertical profiles of atmospheric ions and particles together with atmospheric parameters (temperature, relative humidity and pressure) all along the stratospheric ascent of the BEXUS18 stratospheric balloon. Particles size distributions were measured with the MeteoModem Light Optical Aerosol Counter (LOAC) and air ion density was measured with a set of two commercial and portable ion counters. Though the experimental setup was based upon relatively low-cost and light-weight sensors, vertical profiles of all the parameters up to an altitude of about 27 km were successfully collected. The results obtained are useful for elucidating the relationships between aerosols and charged particles between ground level and the stratosphere with great potential in collecting and adding useful information in this field, also in the stratosphere where such measurements are rare. In particular, the equipment detected coherent vertical profiles for particles and ions, with a particularly strong correlation between negative ions and fine particles, possibly resulting from proposed associations between cosmic rays and ions as previously suggested. In addition, the detection of charged aerosols in the stratosphere is in agreement with the results obtained by a previous flight and with simulations conducted with a stratospheric ion-aerosol model. However, further measurements under stratospheric balloon flights equipped with a similar setup are needed to reach general conclusions on such important issues.


2016 ◽  
Vol 5 (2) ◽  
pp. 437-449 ◽  
Author(s):  
Sindulfo Ayuso ◽  
Juan José Blanco ◽  
José Medina ◽  
Raúl Gómez-Herrero ◽  
Oscar García-Población ◽  
...  

Abstract. Conventional real-time coincidence systems use electronic circuitry to detect coincident pulses (hardware coincidence). In this work, a new concept of coincidence system based on real-time software (software coincidence) is presented. This system is based on the recurrent supervision of the analogue-to-digital converters status, which is described in detail. A prototype has been designed and built using a low-cost development platform. It has been applied to two different experimental sets for cosmic ray muon detection. Experimental muon measurements recorded simultaneously using conventional hardware coincidence and our software coincidence system have been compared, yielding identical results. These measurements have also been validated using simultaneous neutron monitor observations. This new software coincidence system provides remarkable advantages such as higher simplicity of interconnection and adjusting. Thus, our system replaces, at least, three Nuclear Instrument Modules (NIMs) required by conventional coincidence systems, reducing its cost by a factor of 40 and eliminating pulse delay adjustments.


1993 ◽  
Vol 10 (3) ◽  
pp. 211-217 ◽  
Author(s):  
M.L. Duldig ◽  
J.L. Cramp ◽  
J.E. Humble ◽  
J.W. Bieber ◽  
P. Evenson ◽  
...  

Abstract During the solar maximum of 1989–91 an unprecedented sequence of 13 cosmic ray ground-level enhancements (GLEs) was observed by the world-wide neutron monitor network. Of particular interest were two GLEs observed by the Australian network. The 1989 September 29 event was the largest GLE in the space era while the October 22 GLE included an highly anisotropic precursor peak.Analysis of both these GLEs, taking into account disturbed geomagnetic conditions, shows that the particle arrivals at the earth were unusual. The September 29 GLE had significant particle propagation in the reverse direction and as the particle flux decreased following the peak the spectrum also softened. In contrast, the 1989 October 22 precursor exhibited extreme anisotropy while the particles involved in the main GLE showed a complex temporal structure possibly indicating multiple particle injection at the solar acceleration region.


2010 ◽  
Vol 62 (3) ◽  
pp. 333-345 ◽  
Author(s):  
Anja Stadelmann ◽  
Joachim Vogt ◽  
Karl-Heinz Glassmeier ◽  
May-Britt Kallenrode ◽  
Gerd-Hannes Voigt

2019 ◽  
Author(s):  
Xiaochun He ◽  
Carola Butler ◽  
Montgomery Steele ◽  
Sawaiz Syed ◽  
James Shirk ◽  
...  
Keyword(s):  
Low Cost ◽  

2020 ◽  
Author(s):  
Chiara Pinto ◽  
Paola La Rocca ◽  
Davide Nicotra ◽  
Orazio Parasole ◽  
Francesco Riggi
Keyword(s):  
Low Cost ◽  

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