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Table 1.

Nanoflare observations.

Instrument, wavelength Threshold Energies Power-law slope Event frequency References
[Å] [erg] [s−1]

Single-channel detection
SOHO/EIT 304 3σ 1024 − 1027 1.9 ± 0.1 14.4 Berghmans et al. (1998)
SOHO/EIT 195 1024 − 1026 1.35 ± 0.20 1.2
TRACE 171 3σ 1025 − 1027 1.86 ± 0.07 ∼20( * ) Aschwanden & Parnell (2002)
TRACE 195 1.81 ± 0.10 ∼20( * )
TESIS/FET 171 3σ 1023 − 1026 2.79 ± 0.41 Ulyanov et al. (2019b)
2.81 ± 0.52
SDO/AIA 171 3σ 1023 − 1026 2.18 ± 0.20 Ulyanov et al. (2019b)
2.42 ± 0.21
IRIS/SJI 1330, 1400 3σ, 5σ, 7σ 1022 − 1026 < 2 (sunspot) Vilangot Nhalil et al. (2020)
> 2 (plage)
SDO/AIA 171 4σ 1023 − 1024 < 2 ∼100 Chitta et al. (2021)
SOHO/CDS 629.7 3σ 1022 − 1024 2.1 − 3.4 ∼460 Fludra (2023)

Multi-channel detection

3σ 2.59 ∼300( * ) Krucker & Benz (1998)
SOHO/EIT 171, 195 4σ 1025 − 1027 2.54 ∼140( * )
5σ > 2.31 ∼70( * )
TRACE 171, 195 3σ 1024 − 1026 1.79 ± 0.08 ∼5( * ) Aschwanden et al. (2000)
TRACE 171, 195 2σ 1023 − 1026 > 2 ∼800( * ) Parnell & Jupp (2000)
3σ ∼200( * )
SOHO/EIT 171, 195 3σ 1025 − 1027 2.3 ± 0.1 ∼300( * ) Benz & Krucker (2002)
SDO/AIA 2σ 1024 − 1027 1.73 ± 0.01 ∼15( * ) Joulin et al. (2016)
131, 171, 193, 211, 335 1.65 ± 0.02 ∼11( * )
SDO/AIA
94, 131, 171, 193, 211, 335 5σ 1024 − 1029 2.28 ± 0.03 Purkhart & Veronig (2022)

Notes.( * )Our assessment based on the article’s data.

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