If magnetograms or full-disk scans are
used, the original source of files should be indicated.
We would be especially grateful if the authors
sent a short message
with the bibliographic details of their paper when DPD is referred
to.
On the method of compilation of
DPD and its comparative studies see the following papers:
GYÕRI, L.: 1998, Automation
of area measurement of sunspots, Solar Phys.
,180, 109, pdf
BARANYI, T., GYÕRI, L.,
LUDMÁNY, A., Coffey, H.E.: 2001, Comparison of sunspot
area data bases, Monthly Notices of R.A.S., 323(1),
223-230, PDF
GYÕRI, L.:
2003, Compiling sunspot catalogue: the principles, Proc. SIRW
Meeting, (Oct. 23-24, 2003, Royal Observatory of Belgium),
CD-ROM, pdf
GYÕRI, L., BARANYI, T., MURAKÖZY, J.,LUDMÁNY, A.: 2005,Recent
advances in the Debrecen sunspot catalogues, Mem. S.A.It., 76, 981, pdf
GYÕRI, L. : 2005,
Automated determination of the alignment of solar images, Hvar
Obs.
Bull., 29, 299-308, pdf
GYÕRI, L.: 2010, Precise
Determination of the Orientation of the Solar Image, Solar Physics, 267, 445-461, DOI:
10.1007/s11207-010-9663-8
GYÕRI, L.: 2012, Study of differences between sunspot and white light facular area data determined from SDO/HMI and SOHO/MDI observations, Solar Physics, 280, 365-378, DOI: 10.1007/s11207-012-9987-7
BARANYI, T., Király, S., Coffey, H. E.:
2013, Indirect comparison of Debrecen and Greenwich daily sums of sunspot areas, MNRAS, 434 (2), 1713-1720, DOI: 10.1093/mnras/stt1134, PDF preprint