目的探究护理干预对慢性阻塞性肺疾病（COPD）患者使用舒利迭吸入剂的影响。方法选取我院呼吸内科2010年1月～2012年1月期间收治的COPD患者80例分为观察组和对照组，每组40例，两组患者均接受舒利迭吸入剂治疗。在此基础上观察组由专职...目的探究护理干预对慢性阻塞性肺疾病（COPD）患者使用舒利迭吸入剂的影响。方法选取我院呼吸内科2010年1月～2012年1月期间收治的COPD患者80例分为观察组和对照组，每组40例，两组患者均接受舒利迭吸入剂治疗。在此基础上观察组由专职护士给予护理干预。比较两组患者吸入方法的掌握情况、COPD急性发作率以及生活质量（quality of life，QOL）评分，评价干预措施对治疗的影响。结果观察组吸入方法的正确掌握率明显高于对照组，而COPD急性发作率显著低于对照组，观察组心理功能、躯体功能和社会功能的评分都高于对照组，差异均具有统计学意义（P〈0．05）。结论对COPD患者的护理干预可提高舒利迭的正确使用率和患者自我管理依从性，改善患者病情，降低急性发作率，提高患者的生活质量，效果显著。展开更多
We present a brief overview of follow-up observations of GRB afterglows made by the 0.8-m TNT and other telescopes at the Xinglong observatory during the last three years.Our system,dedicated to the measurement of ear...We present a brief overview of follow-up observations of GRB afterglows made by the 0.8-m TNT and other telescopes at the Xinglong observatory during the last three years.Our system,dedicated to the measurement of early-time optical afterglow emission,responded to 50 GRBs from Jan.2006 to Apr.2009.Among them,about 50% have been successfully detected.The fastest response time is 76 sec(GRB 061110A and GRB 090426) after the space-borne GRB detector was triggered.The redshift distribution spans the range from z = 0.033(GRB 060218) to z = 5.6(GRB 060927).We also report the optical photometric follow-up of GRB 080330,which is an X-ray flash,as an example of our observations.展开更多
文摘目的探究护理干预对慢性阻塞性肺疾病（COPD）患者使用舒利迭吸入剂的影响。方法选取我院呼吸内科2010年1月～2012年1月期间收治的COPD患者80例分为观察组和对照组，每组40例，两组患者均接受舒利迭吸入剂治疗。在此基础上观察组由专职护士给予护理干预。比较两组患者吸入方法的掌握情况、COPD急性发作率以及生活质量（quality of life，QOL）评分，评价干预措施对治疗的影响。结果观察组吸入方法的正确掌握率明显高于对照组，而COPD急性发作率显著低于对照组，观察组心理功能、躯体功能和社会功能的评分都高于对照组，差异均具有统计学意义（P〈0．05）。结论对COPD患者的护理干预可提高舒利迭的正确使用率和患者自我管理依从性，改善患者病情，降低急性发作率，提高患者的生活质量，效果显著。
基金supported by the National Basic Research Program of China (Grant No. 2009CB824800)the National Natural Science Foundation of China (Grant Nos. 10673014 and 10803008)
文摘We present a brief overview of follow-up observations of GRB afterglows made by the 0.8-m TNT and other telescopes at the Xinglong observatory during the last three years.Our system,dedicated to the measurement of early-time optical afterglow emission,responded to 50 GRBs from Jan.2006 to Apr.2009.Among them,about 50% have been successfully detected.The fastest response time is 76 sec(GRB 061110A and GRB 090426) after the space-borne GRB detector was triggered.The redshift distribution spans the range from z = 0.033(GRB 060218) to z = 5.6(GRB 060927).We also report the optical photometric follow-up of GRB 080330,which is an X-ray flash,as an example of our observations.
