Cosmic ray physics with the TRAGALDABAS detector
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1 Cosmic ray physics with the TRAGALDABAS detector Juan A. Garzón LabCAF, IGFAE. Univ. Santiago de Compostela on behalf of the TRAGALDABAS Collaboration ISCRA. Moscow, 1 June 22nd. 2017
2 Outlook: 1. The beginning 2. The TRASGO 3. The first TRASGO: TRAGALDABAS 4. TRAGALDABAS: preliminary results - FD June Atmosphere analysis 5. The TRASGO : Next steps & Summary ISCRA. Moscow, 2 June 22nd. 2017
3 The beginning The Nuclear Physics HADES experiment The RPC wall commissioning The HADES spectrometer at GSI-Darmstadt RPC commissioning with cosmic rays 3
4 The beginning A cosmic ray shower picture using the HADES RPC detectors δt ~ 150 ps, δs ~ 5 cm 2, δθ ~5º Never cosmic rays were observed at the Earth s surface with such accuracy! 4
5 The TRASGO project The idea: why not developing modular cosmic ray tracking detectors? The solution: TRASGO (= pixie, goblin) : TRAck reconstructing box - Multi-channel Tracking detector - Modular concept - Sensitive to both muon and electromagnetic showers (software PID) - Stand-alone Plug&Play very affordable detector (RPC-based) 5
6 The first Trasgo: TRAGALDABAS (Pronuntiation: truguldubus) TRAsGo for the AnaLysis of the nuclear matter Decay, the Atmosphere, the earth B-field And the Solar activity 6
7 The first Trasgo: TRAGALDABAS The TRAGALDABAS Collaboration H. Alvarez-Pol, A.Blanco, J.J.Blanco, P.Cabanelas, J.Collazo, J.Cuenca, P.Fonte, Y.Fontenla, D.García Castro, J.A.Garzón, A.Gómez-Tato, D.González-Díaz, G.Kornakov, T.Kurtukian, L.Lopes, A.Morozova, J.C.Mouriño, M.A.Pais, A.Pazos, V.Pérez Muñuzuri, P.Rey, I.Riádigos, M.Seco, V. Villasante Laboratory / Task 1. Univ. Alcalá de Henares, Spain / Solar Physics 2. CEN - Bordeaux, France / Nuclear and Solar Physics 3. CITEUC - U. Coimbra, Portugal / Geomagnetic field and Space Weather 4. CESGA Supercomputation Center - Santiago de Compostela, Spain / Data storage and distribution 5. GENP - Univ. Santiago de Compostela, Spain / Software development and simulation 6. IGFAE - Univ. Santiago de Compostela, Spain / Monitoring and Slow control 7. LabCAF - Univ. Santiago de Compostela, Spain / Track reconstruction and data analysis 8. NLFG - Univ. Santiago de Compostela, Spain / Atmosphere and Climate studies ATI Sistemas. La Coruña, Spain Hydra Technologies Spain S.L. Vigo, Spain Club Desarrollo de las Ciencias, Madrid, Spain Other partners: 7
8 The first Trasgo: TRAGALDABAS Location 8
9 The first Trasgo: TRAGALDABAS The site Location: Fac. Physics Univ. Santiago de Compostela N: 42º52 34, W: 8º
10 The first Trasgo: TRAGALDABAS The timing RPC technology Main features: - Very affordable technology - Very good time resolution: ~0.5 ps (10x12) channels (~11x11 cm 2 ) m 2 (1.2 x 1.5 m 2 ) planes 10
11 The first Trasgo: TRAGALDABAS PID capability Plane T1 Plane T2 Plane T4 11
12 The first Trasgo: TRAGALDABAS PID capability Range: Electrons Range: Gammas Electrons. Radial Dispersion in layers Gamma. Radial dispersion in layers > [ cm ] σ r < nd 2 layer rd 3 layer th 4 layer > [ cm ] σ r < nd 2 layer rd 3 layer th 4 layer E [ GeV ] Gamma showers are broader than electron showers E [ GeV ] 12
13 The first Trasgo: TRAGALDABAS EnsarRoot based detector simulation 13
14 The first Trasgo: TRAGALDABAS Tracking strategies based on TimTrack data, d timtrack (X0, X, Y0, Y T0, V) parameters + fitting models: m zi (xi,yi,ti) Method 1. xi = X0 + X zi yi = Y0 + Y zi ti = T0 + V1+X 2 +Y 2 zi / V Direct fit to 6 parameters! Z Method 2. We are trying to implement a new method including the drift time of electrons in the electrodes. Still, convergence problems! :( 14
15 TRAGALDABAS: preliminary results Data sample: fired cells map Plane T1 Plane T2 Plane T4 DOY 2015 DOY 2016 DOY years of data collected: ~ events! 15
16 TRAGALDABAS: preliminary results Trigger summary Trigger rate: ~ 70 Hz. Event rate: ~ 7Mevents /day Storage rate: ~ 0.7 Tb / year (1.9 Gb /day) Mean duty time: > 90% 16
17 TRAGALDABAS: preliminary results 2 year rate behaviour (pressure corrected) Multiplicity M=1 Multiplicity M=2? Multiplicity M=3? Multiplicity M=4 Multiplicity M>4 17
18 TRAGALDABAS: preliminary results Preliminary reconstructed data sample (Lower energy) (Higher energy) 18
19 TRAGALDABAS: preliminary results CME SOHO satellite picture. 2015, June 21st Analysis of the FD of June 2015 FD Interesting excesses! 19
20 TRAGALDABAS: preliminary results CME SOHO satellite picture. 2015, June 21st Analysis of the FD of June 2015 FD is observed very well with a roughly 2 m 2 detector! 20
21 TRAGALDABAS: preliminary results Analysis of the FD of June 2015 sh1 sh2 /Jun21 /Jun23 /Jun25 Interesting feature: high multiplicity excesses seem to be associated with the first magnetic shock! 21
22 TRAGALDABAS: preliminary results Atmosphere slope analysis Slopes of linear fits of the relative rate changes (dr/r) as a function of the relative temperature changes (dt/t) at different pressure levels 22
23 TRAGALDABAS: preliminary results Atmosphere slope analysis Slopes: Rate - Temperature Troposphere Tropopause Stratosphere Sea level Different multiplicity (energy) events show a different behaviour respect temperatures at the different heights of the atmosphere 23
24 TRAGALDABAS: preliminary results Atmosphere slope analysis Slopes: Rate - Temperature ICE CUBE Troposphere Tropopause ICE TOP Stratosphere Sea level We observe similar trends that the ones observed in the IceTop - IceCube observatory for low and high energy muons 24
25 The TRASGO proyect: next steps - Install new Trasgos in other places: Vigo & Spanish Antarctic Base TRAGALDABAS S. Compostela Vigo TRITON South Atlantic Magnetic Anomaly CRay data will be taken during the journey in the ship Hesperides Antartida-2018 TRISTAN ISCRA. Moscow, 25 June 22nd. 2017
26 The TRASGO proyect: next steps - Install new Trasgos in other places: Vigo & Spanish Antartic Base TRISTAN Neutron Monitors ORCA: Observatorio de Rayos Cósmicos Antártico ISCRA. Moscow, 26 June 22nd. 2017
27 The TRASGO proyect: next steps - Install four SALLA radio-antennas provided by KIT (Karlsruhe), on the roof for identifying high energy air showers. - ISCRA. Moscow, 27 June 22nd. 2017
28 The TRASGO proyect: next steps - Look for new signatures allowing a better measurement of primary cosmic rays ISCRA. Moscow, 28 June 22nd. 2017
29 Summary - TRASGOS are very interesting devices that may allow us to improve significantly our knowledge on many cosmic rays aspects. - Preliminary results are very encouraging - TRASGOS are complicated devices and still several problems should be fixed - A first detector is operative and taking data regularly at the Univ. of Santiago de Compostela. Soon other TRASGOS will be operative in other places providing new data 29
30 the end Thanks! 30
31 TRAGALDABAS: preliminary results Analysis of the FD of November 2015 Nov. 3rd. TRAGALDABAS M= 1 Nov. 3rd. TRAGALDABAS M= 2 Nov. 3rd. TRAGALDABAS M= 3 Nov. 7th. Nov. 7th. Nov. 7th. Nov. 3rd. TRAGALDABAS M= 4 Nov. 3rd. TRAGALDABAS M> 4 Nov. 7th. Nov. 7th. Nov. 7th. Oulu Nov15 31
32 TRAGALDABAS: preliminary results Analysis of the FD of November 2015 Nov. 3rd. TRAGALDABAS M= 1 Nov. 3rd. TRAGALDABAS M= 2 Nov. 7th. Nov. 7th. Nov. 3rd. TRAGALDABAS M= 3 Nov. 3rd. TRAGALDABAS M> 4 Nov. 7th. Nov. 7th. 32
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