作者: filicide 時間: 2025-3-21 22:51 作者: 偏離 時間: 2025-3-22 03:37
DrugsThe choice of an opioid for spinal administration is based not only on pharmacokinetics but also on some criteria of unequal importance:作者: Ceremony 時間: 2025-3-22 06:39 作者: evaculate 時間: 2025-3-22 12:12
Intraoperative useSpinal opioids (with the exception of high doses of intrathecal pethidine) are not able to provide surgical anaesthesia. Nevertheless, they can be used peroperatively in two situations.作者: Lipoprotein(A) 時間: 2025-3-22 14:29 作者: 揉雜 時間: 2025-3-22 20:17 作者: 別炫耀 時間: 2025-3-22 23:30
Cancer painPain is experienced by 60 to 85% of patients with terminal carcinoma and requires effective and consistent therapy (Bonica 1987).作者: Substance-Abuse 時間: 2025-3-23 03:18
Perineural opioid analgesia (PNOA)After the good analgesic results obtained with the epidural, intrathecal or intra-cerebroventricular adminstration of opioids, some authors have made an attempt to administer opioids by the perineural route, especially for pain treatment of the extremities.作者: Corral 時間: 2025-3-23 09:35
Developments in Critical Care Medicine and Anaesthesiologyhttp://image.papertrans.cn/r/image/825347.jpg作者: SLAG 時間: 2025-3-23 10:51
https://doi.org/10.1007/978-94-009-2321-8Infusion; Trauma; care; central nervous system; complications; infection; intensive care; intensive care un作者: curriculum 時間: 2025-3-23 15:27
Pharmacokinetics of opioidsoids (Casy 1971). However, pharmacokinetic factors display striking differences: e.g. molecular weight, lipid solubility, protein binding, ionization, influence the action of opioids, increase or decrease the transport across membranes, the receptor binding affinity, the diffusion into the CNS, the analgesic action, etc. (Tab. 11, 12).作者: 加入 時間: 2025-3-23 21:04 作者: 情愛 時間: 2025-3-23 22:46
Side effectsratory, urinary, neuromuscular, gastro-intestinal and sexual functions may also occur. They demonstrate an occurrence in relationship to the segmental progression of analgesia and rostral spread of the opioid.作者: 燒瓶 時間: 2025-3-24 05:06 作者: choleretic 時間: 2025-3-24 09:20
Chronic non-malignant painr patients with non-cancer related chronic pain (Harbaugh 1983). This is generally the case if social and psychological factors (anxiety, opioid abuse, insecurity, etc.) play a greater role in pain perception than ongoing tissue injury.作者: neuron 時間: 2025-3-24 12:57
978-94-010-7543-5Kluwer Academic Publishers 1991作者: 有特色 時間: 2025-3-24 17:53 作者: abreast 時間: 2025-3-24 22:39
Book 1991pioids are minute as compared to morphine and meperidine. Regional Opioid Analgesia could not have been more authentically written than by Drs. De Castro,Zenz and Meynadier,who have conducted daily clinical investigations on all known opioids for regional analgesia as well as for neurolept analgesia作者: 全面 時間: 2025-3-25 02:57 作者: concert 時間: 2025-3-25 05:22 作者: 名字 時間: 2025-3-25 09:06
ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: Muscularis 時間: 2025-3-25 15:12 作者: chemoprevention 時間: 2025-3-25 18:32
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: Digest 時間: 2025-3-25 23:33 作者: 不透明性 時間: 2025-3-26 00:18
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: MUMP 時間: 2025-3-26 05:23
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: 束縛 時間: 2025-3-26 12:04
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: 有其法作用 時間: 2025-3-26 13:28 作者: growth-factor 時間: 2025-3-26 20:01
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: IRS 時間: 2025-3-27 00:53
ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: 改變立場 時間: 2025-3-27 01:21 作者: chondromalacia 時間: 2025-3-27 06:26 作者: 心胸開闊 時間: 2025-3-27 13:23 作者: Intentional 時間: 2025-3-27 14:10
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.作者: insurgent 時間: 2025-3-27 21:02
0924-5294 rs. De Castro,Zenz and Meynadier,who have conducted daily clinical investigations on all known opioids for regional analgesia as well as for neurolept analgesia978-94-010-7543-5978-94-009-2321-8Series ISSN 0924-5294 作者: 光滑 時間: 2025-3-27 22:31
th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: OUTRE 時間: 2025-3-28 05:58 作者: insert 時間: 2025-3-28 06:20 作者: motivate 時間: 2025-3-28 11:51
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: 招待 時間: 2025-3-28 14:36
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: 平息 時間: 2025-3-28 22:14
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: 向下 時間: 2025-3-29 01:04
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: Wordlist 時間: 2025-3-29 06:35
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: 剛開始 時間: 2025-3-29 10:13
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: Atrium 時間: 2025-3-29 13:58
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: Acupressure 時間: 2025-3-29 18:23 作者: 裝飾 時間: 2025-3-29 21:38 作者: Outspoken 時間: 2025-3-30 03:34 作者: limber 時間: 2025-3-30 05:24
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: 表示向前 時間: 2025-3-30 11:46
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: 手勢 時間: 2025-3-30 13:52
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu作者: Homocystinuria 時間: 2025-3-30 17:33
Anatomy and physiologyed stimuli we can distinguish between nociceptors, mechanoreceptors, thermoreceptors and polymodal receptors. Nociceptors are distributed over the whole body from the skin surface to the viscera (Fig. 3, 4, 5, 6).作者: craving 時間: 2025-3-30 22:42
Introductionly, the historical development and rapid application of spinal opioids provide emphatic support for the premise that: a fundamental appreciation of the mechanisms by which the nervous system processes sensory information represents the principle route by which rational advances in pain therapy will occur.作者: machination 時間: 2025-3-31 01:09
Book 1991by the authors to write a preface to this monumental monograph, Regional Opioid Analgesia. Regional Opioid Analgesia is a colossal undertaking by Drs. De Castro, Meynadier and Zenz shortly after the introduction of this revolutionary approach to pain relief which opened a new epoch in analgesiology.作者: CHAR 時間: 2025-3-31 08:48 作者: chiropractor 時間: 2025-3-31 10:31 作者: Dedication 時間: 2025-3-31 14:27
Pharmacokinetics of opioidsoids (Casy 1971). However, pharmacokinetic factors display striking differences: e.g. molecular weight, lipid solubility, protein binding, ionization, influence the action of opioids, increase or decrease the transport across membranes, the receptor binding affinity, the diffusion into the CNS, the 作者: Limousine 時間: 2025-3-31 21:30
Pharmacodynamics of opioidsd interactions of spinal opioids are those with the spinal receptors. But rostral distribution and effect on brain receptors as a source of undesired actions can neither be completely prevented nor completely excluded.作者: 不公開 時間: 2025-3-31 22:53
Side effectsratory, urinary, neuromuscular, gastro-intestinal and sexual functions may also occur. They demonstrate an occurrence in relationship to the segmental progression of analgesia and rostral spread of the opioid.
