This file is about the data rectification procedure and its details. Almost all data sets were underwent a procedure of the manual rectification with the use of a special graphically-interactive software tool. This rectification has been performed just to make the data, as most as possible, free of the unreliable data. The people who knows the instrument and other conditions of the experiment were involved in this work for the most authoritative judging. No changes in the data were made, only throwing. In addition to the basic procedure of rectification, the second level of rectification has been performed in several cases. So, there are two following levels of rectification: - at the 1st level of rectification all obviously unreliable values are being thrown, only; - at the 2nd level of rectification most of values being suspected as unreliable (noisy) are being thrown. The results of the 1st level of rectification are placed in the main spacecraft-specific directory. If the 2nd level of rectification is performed, its results are placed in a subdirectory /lownoise. Concerning usage of both data files, the data in the main directory are most suitable for detailed and non-automated analysis since some intervals with noisy data in some channels (lower energies and sunward direction) might be left there. If one wants to perform the automated data analysis for studying some large-scale effects, it is better to use the contents of a /lownoise subdirectory. Please note that the additional rectification has not been performed for all data sets from the TASPD SINP MSU collection. Some files do not need this, but some groups of data from GRANAT, for example, should be probably processed this way yet.