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@ARTICLE{Walter:619087,
      author       = {Walter, Michael and Gnebner, C. and Heber, B. and Herbst,
                      K. and Krüger, H. and Krüger, H. G. and Kühl, P. and
                      Prokoph, H. P. and Strauss, R. D.},
      title        = {{M}easurements of {C}osmic {R}ays by a {M}ini‐{N}eutron
                      {M}onitor at {N}eumayer {III} {F}rom 2014 to 2017},
      journal      = {Space weather},
      volume       = {22},
      number       = {6},
      issn         = {1542-7390},
      address      = {[New York]},
      publisher    = {Wiley},
      reportid     = {PUBDB-2024-07374},
      pages        = {e2023SW003596},
      year         = {2024},
      abstract     = {A mini-neutron monitor (MNM) was installed at the German
                      Antarctic Neumayer III station, measuring the variation of
                      galactic cosmic rays and searching for Forbush Decreases
                      (FDs) caused by solar activities. Running continuously from
                      2014 until the end of 2017, the long-term stability of the
                      detector could be investigated. After correcting the air
                      pressure and normalization to the 27 days running mean
                      averages of the SANAE and TERA Neutron Monitors (NMs), the
                      daily running mean count rates are compared with the SANAE
                      and TERA NMs also installed in Antarctica. For most of the
                      14 FDs with magnitudes greater than 3, taken from the list
                      compiled by the IZMIRAN group
                      (http://spaceweather.izmiran.ru/eng/dbs.html), the three
                      detectors show consistent particle flux variation, although
                      the average rate of the MNM is more than a hundred times
                      smaller. The light and low-cost MNM is an ideal alternative
                      to heavy and old NMs, especially at high altitudes and
                      remote environments.},
      cin          = {$Z_KOM$},
      ddc          = {550},
      cid          = {$I:(DE-H253)Z_KOM-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)CTA-20150101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:001241763700001},
      doi          = {10.1029/2023SW003596},
      url          = {https://bib-pubdb1.desy.de/record/619087},
}